The galaxy presents a generally smooth and rounded morphology. It exhibits a dominant central bulge with a somewhat diffuse profile, suggesting an older stellar population. The color appears yellowish, which is also consistent with an older stellar population and potentially a lower rate of ongoing star formation.

There is a possible secondary component or companion galaxy located close to the primary galaxy. This object appears smaller and slightly less luminous than the primary galaxy. It is not certain whether this is an interacting galaxy or a separate object located along a similar line of sight. The image quality does not allow to confirm any tidal distortions or bridges.
