The galaxy presents as a concentrated, moderately bright object with an elliptical morphology. It displays a significant central bulge, characterized by a prominent yellowish hue, indicative of an older stellar population. Extending outwards from the core, there's a diffuse, less luminous disk component with a slightly bluer tint. This suggests the presence of some ongoing star formation, albeit at a relatively low rate. The galaxy appears largely undisturbed, showing no strong signs of tidal interactions or recent major mergers, though there are hints of minor irregularities in the outer regions. Its overall structure suggests a system transitioning towards a more quiescent state.