The galaxy presents as a relatively smooth object with a dominant, bright central bulge. The overall shape appears elliptical or lenticular, lacking the distinct spiral arm structure often observed in disk galaxies. There is a slight elongation present, but it is closer to round than cigar shaped. The color gradient suggests an older stellar population, with a yellowish-red hue more prevalent in the central regions, indicating a diminished rate of recent star formation. There is no evidence of a significant ongoing merger or tidal disruption. The galaxy appears mostly undisturbed, lacking any prominent distortions or asymmetries in its overall structure. 
