The galaxy appears to be elliptical in shape, exhibiting a smooth and largely featureless morphology. The light profile suggests a centrally concentrated bulge, with a gradual decrease in luminosity outwards from the core. The color is predominantly yellowish-white, indicative of an older stellar population. There is no readily apparent disk structure or spiral arm formation. There appears to be no ongoing major merger activity. There is also no sign of substantial dust lanes or significant star formation regions. Overall, the object is consistent with a relatively quiescent elliptical galaxy with a high degree of symmetry.
