The galaxy presents as a moderately bright, relatively smooth, oval-shaped structure, consistent with an elliptical or lenticular type. The central region exhibits a high surface brightness, indicating a dense concentration of stars. A subtle color gradient is observed, with the core appearing more yellow/orange, potentially suggestive of an older stellar population. The outer regions fade gradually into the background, displaying a bluer hue possibly resulting from ongoing low-level star formation activity. There is a slight indication of a faint, extended disk-like component oriented roughly horizontally. The galaxy seems to be largely undisturbed, showing no obvious signs of recent major mergers or strong tidal interactions, although a minor disturbance may be present.
