The galaxy presents as an elliptical system with a smooth, concentrated light profile. Its core exhibits a bright, yellowish-white hue, suggesting a population of older stars and a minimal amount of dust obscuration in the central region.

The galaxy's overall shape is elongated, appearing oval. There is no prominent spiral arm structure or distinct features indicative of active star formation. The galaxy fades gradually toward its outer edges, with a slight bluer tinge compared to the core. The outer regions are smoother, indicating an older stellar population and a lack of significant dust lanes or gas clouds. 

No tidal tails, obvious signs of recent mergers, or active galactic nuclei are apparent in this image.
