The galaxy appears to be an elliptical, or possibly lenticular, galaxy. Its light is generally smooth and concentrated towards the center, with a slight elongation suggesting a cigar shape. While the galaxy lacks distinct spiral arms, the light distribution is not perfectly uniform. Some irregularity hints that it is not a perfectly smooth spheroid, and that it has potentially experienced recent disturbance events.

The color gradient indicates an older stellar population dominating the galaxy's composition. The core of the galaxy is a yellower hue, indicating a likely abundance of older, cooler stars, while the outer regions appear somewhat bluer, which could be due to a small amount of ongoing star formation activity in the galaxy's outer regions. This small amount of star formation is reflected in its luminosity, which suggests some gas and dust is still present.

The morphology does not show any obvious signs of a major merger event, though minor disturbances appear to be present. Based on the absence of strong tidal tails, if a merger has taken place, it was likely some time ago or of low mass ratio. The galaxy does not appear to be actively interacting with other nearby galaxies currently.
