The galaxy presents a generally smooth, elliptical morphology. The central bulge is pronounced and exhibits a bright, concentrated luminosity, suggesting a high stellar density and potentially an older stellar population. The color of the bulge appears slightly yellowish-white. There is evidence of a surrounding, fainter disk. This disk appears relatively featureless, displaying a gradual decline in surface brightness with increasing radial distance from the core. The shape of the galaxy tends towards a more rounded form with a slight elongation. There is no immediately apparent evidence of significant tidal disturbances, ongoing major mergers, or prominent dust lanes. The overall impression is of a relatively evolved system, potentially an early-type spiral or lenticular galaxy, undergoing quiescent star formation.
