The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. The light is centrally concentrated, with a gradual decrease in luminosity outwards. There is little evidence of spiral arms or a distinct disk structure.

The galaxy exhibits a yellowish-white hue, consistent with an older stellar population. There does not appear to be an abundance of dust lanes or regions of active star formation within the galaxy. However, there are some signs of some disturbed features or perhaps an interaction with a smaller nearby galaxy, and potential merging activity is present.
