The galaxy presents as a primarily smooth, elliptical-like structure. It exhibits a concentrated central bulge, appearing yellowish-orange in color, which suggests an older stellar population. The overall shape leans toward being somewhat elongated. There are subtle hints of a fainter, more diffuse outer halo or envelope surrounding the central region, displaying a bluer color. This could be indicative of some low-level ongoing star formation. No significant tidal disturbances or signs of major mergers are immediately apparent, although there appears to be minor disturbance surrounding the halo, warranting further investigation.
