The galaxy presents as an elliptical-like morphology, exhibiting a centrally concentrated bulge surrounded by a fainter, more diffuse halo. The central region displays a yellowish-orange hue, suggestive of an older stellar population. A bluer color is present in the halo, possibly indicating some star formation activity. The galaxy appears relatively smooth, with only subtle variations in surface brightness. Faint features suggesting minor disturbances are present, but the overall structure does not indicate a major ongoing merger.
