The galaxy exhibits a generally elliptical morphology, displaying a smooth appearance with a dominant, centralized bulge. The color profile is generally redder, suggesting an older stellar population and/or significant dust content. There may be faint tidal features present or a very faint disk, indicated by subtle asymmetries in the light distribution, although the galaxy is largely spheroidal. There is a strong central core of light, suggesting a large supermassive black hole.

Overall, the galaxy is most likely a large, quiescent elliptical galaxy at an approximate distance corresponding to a redshift of ~0.3. There is a good likelihood of a recent merger, but not a major one.
