The galaxy presents a predominantly smooth morphology, appearing as an elliptical or lenticular type. Its shape approximates an oblate spheroid, with a slight elongation. There is a bright, centrally concentrated bulge region that dominates the galaxy's luminosity profile. The light appears relatively uniform across the galaxy, with only subtle color variations. The inner regions exhibit a yellowish or gold hue, possibly indicative of an older stellar population. Fainter, diffuse bluish light can be observed in the outskirts, suggesting the presence of some younger stars or residual star formation. There is no evidence of prominent spiral arms, bars, or other significant disk features. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers. There are subtle asymmetries in the galaxy's outer isophotes, potentially indicating minor past interactions. Overall, this galaxy appears to be a massive, evolved system with a dominant bulge component and a relatively quiescent star formation history.
