The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical morphology, appearing largely rounded in shape. The galaxy's light profile suggests a dominant bulge component, with a gradual decrease in luminosity towards the outer regions. There's a hint of a disk-like structure. The color appears to be predominantly yellow-white, potentially indicating a population of older stars. There is no readily discernible evidence of ongoing major merger activity or significant tidal disturbances. The overall structure suggests a classification leaning towards an early-type spiral or possibly a lenticular galaxy.
