The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. A dominant, bright central bulge is apparent, with a gradual decrease in luminosity moving outwards. There is little to no evidence of spiral arm structures or dust lanes. The color profile suggests an older stellar population. Subtle irregular extensions are present in the surrounding halo, hinting at possible past minor interactions. Overall, this galaxy appears to be an elliptical galaxy with low star formation activity and a significant spheroidal component.
