The galaxy presents as an elliptical morphology, displaying a smooth, diffuse light distribution. There is a strong central concentration of light, indicative of a prominent nucleus. The galaxy exhibits a yellowish-orange hue, suggesting a population dominated by older stars. The overall shape appears largely spheroidal, with a slight deviation toward an intermediate ellipticity. No distinct features such as spiral arms, dust lanes, or tidal tails are discernible. The galaxy appears relatively isolated, with no apparent signs of recent or ongoing major merger activity, though subtle disturbances cannot be ruled out entirely.
