The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions outward into a less defined, diffuse halo. The light distribution suggests a relatively old stellar population, contributing to its reddish-yellow hue. The galaxy appears to be relatively isolated, showing no obvious signs of tidal interactions or recent major mergers, though a minor disturbance in its form is possible. The overall color profile indicates a lack of significant recent star formation activity. It is moderately luminous, exhibiting a substantial mass estimate. The structure appears to be more 'in between' being round or elliptical.
