The galaxy exhibits an elliptical morphology, appearing largely spheroidal with a smooth light profile and a centrally concentrated bulge. There is a slight extension to one side, suggesting a possible tidal feature or minor disturbance. The dominant color is a yellow-white hue, indicating a population of older stars with a lower rate of star formation. There appears to be little evidence of dust lanes or spiral arm structures. There are no signs of a strong ongoing merger, although some gravitational disturbance cannot be ruled out.
