The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that dominates the light profile. There is little evidence of spiral arms or significant disk structure, and the galaxy appears largely spheroidal. Coloration suggests an older stellar population, with a yellowish-red hue indicative of evolved stars. The galaxy shows a fairly homogenous luminosity distribution across its body, with the exception of the bright central bulge. There are no strong indications of ongoing major mergers or tidal disturbances, although there could be some minor asymmetries. Overall, this galaxy appears to be a relatively quiescent, early-type system.
