The galaxy appears as a largely featureless, elliptical-type system. It exhibits a centrally concentrated luminosity profile, with the light intensity decreasing gradually from the core outwards. The color appears generally yellow, suggesting a population of older stars and a relatively low rate of ongoing star formation. There is no clear evidence of spiral arms, a central bar, or significant dust lanes. The overall shape is quite circular, indicating a minimal degree of flattening. The galaxy appears isolated, with no obvious signs of tidal interaction or recent merging events, though some minor disturbance cannot be ruled out.
