The galaxy presents a primarily smooth morphology, suggestive of an elliptical or lenticular type. It exhibits a concentrated central bulge that is relatively bright, with a gradual decrease in luminosity towards the outer regions. The galaxy's overall shape appears somewhat elongated, exhibiting an intermediate ellipticity between round and cigar-shaped. No prominent spiral arms or distinct disk structures are discernible in this image. There is no visual evidence of ongoing major mergers or significant tidal disturbances. There is a slight color gradient, with the central bulge appearing more yellow/orange, potentially indicating an older stellar population. The outer regions appear slightly bluer, which could imply the presence of younger stars, but this is very subtle.
