The galaxy presents as a largely smooth, elliptical-type morphology. Its light profile appears centrally concentrated, with a bright, yellowish core that fades gradually outwards. No distinct spiral arm structures or prominent dust lanes are discernible. The galaxy appears relatively isolated, without obvious signs of tidal interactions or major disturbances that would indicate a recent merger event. A very slight ellipticity is observed with a possible hint of a disk. The overall color suggests a population dominated by older stars, consistent with a low specific star formation rate.
