This galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It has a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The galaxy exhibits a slightly elongated shape, deviating somewhat from a perfect sphere. The color profile suggests a generally older stellar population, with the central regions appearing brighter. The galaxy does not show any obvious signs of spiral arms or significant dust lanes. There is no evidence of any major mergers or tidal disturbances, although a slight asymmetry in the outer halo may indicate a minor past interaction or accretion event. Overall, this galaxy presents as a well-formed, mature system with a generally smooth morphology.
