The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile. The central region is bright and yellowish, with a gradual decrease in luminosity towards the outer edges. There is a slight elongation, with a roughly round shape. No spiral arm structures or prominent dust lanes are visible. The lack of distinct features suggests a relatively old stellar population and a low rate of current star formation. There is no obvious sign of any recent or ongoing major mergers or tidal disturbances. The morphology suggests a galaxy that has largely settled into a stable configuration.
