The galaxy appears as a relatively smooth, centrally concentrated object with an elliptical morphology. Its color profile exhibits a gradual reddening towards the center, indicative of an aging stellar population and/or increased dust concentration. The outer regions of the galaxy display a bluer hue, which may point to younger stars. A faint disc might be present, with a near face-on orientation. No spiral arm structures are evident, and there are no obvious signs of strong tidal interactions or recent major merger events. Minor irregularities or disturbances cannot be entirely ruled out.
