The galaxy presents an elliptical morphology, displaying a smooth, concentrated light profile. The central bulge appears bright and yellow, indicative of an older stellar population. The galaxy's light falls off gradually from the core, showing a distinct lack of spiral arm structure. The overall shape is slightly elongated, but notably round, deviating only subtly from a perfect circle. There are no visible signs of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy. Faint, diffuse extensions of light are not easily discernible, suggesting minimal recent star formation. The galaxy appears to be relatively isolated within its field of view, showing no signs of interacting companions.
