The galaxy exhibits a generally elliptical morphology in projection. The central region displays a bright, concentrated core that appears relatively smooth. There are faint extensions or diffuse features emanating from the central region, with some evidence of non-uniformity in the outer structure. The color profile suggests variations, with a bluer hue concentrated toward the center and a gradual shift towards redder colors in the outer regions. These color variations may indicate differences in stellar populations or dust content within the galaxy. There is a possible indication of minor disturbance. Overall, the galaxy appears to be relatively isolated with no immediately apparent tidal features or close companion galaxies.
