The galaxy appears as a luminous, elliptical structure with a relatively smooth profile. The central region exhibits a concentrated, yellowish-white hue, indicative of an older stellar population. Fainter, diffuse extensions of the galaxy are visible, particularly towards what appears to be the right of the central bulge. These extensions exhibit a slightly bluer tint compared to the core, possibly suggestive of more recent star formation activity. Irregularities in the galaxy's shape hints it might be a late-stage merger or experiencing minor disturbances.