The galaxy presents as a centrally concentrated, smooth object with an overall elliptical morphology. The core region displays a yellowish hue, suggesting a population of older stars. Fainter, diffuse extensions are observed beyond the core, transitioning into a reddish color. This could indicate a less concentrated population of older stars within the galaxy's halo. The lack of prominent spiral arms or strong dust lanes suggests an early-type galaxy, potentially an elliptical or lenticular. There is a slight elongation of the galaxy along one axis, but no obvious signs of tidal disturbances or ongoing major merging events are detected in the image. There are a couple regions of faint blueish light located further from the central core, possibly indication of some localized star formation.
