The galaxy presents a relatively smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in brightness from the core outwards. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a yellowish-white hue in its central region, suggesting a population of older stars. The outer regions are slightly bluer, potentially indicating the presence of younger stars, though the overall star formation rate appears to be low. There is no obvious evidence of significant tidal disturbances or ongoing merger activity, and the galaxy's shape tends more towards a flattened ellipse.
