The galaxy presents as an elliptical morphology, with a smooth light distribution and no discernible spiral arm structure. The central bulge exhibits a concentrated, yellowish-white hue, suggestive of an older stellar population. Moving outwards, the color gradually shifts towards a bluish halo, which could indicate the presence of some younger stars and ongoing, but low-level, star formation. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions. There is a slight asymmetry in the outer regions which could indicate some kind of interaction, but it is not conclusive. Overall, the galaxy appears to be a reasonably massive system, with a centrally concentrated profile.
