The galaxy appears as a somewhat elliptical, centrally concentrated object. The light profile exhibits a smooth gradient, with the highest intensity emanating from the core region. The overall color suggests an older stellar population, with a yellowish hue dominating. There is a slight asymmetry visible in the outer regions, possibly indicating a minor gravitational disturbance or interaction, though no distinct tidal features or signs of a major merger are immediately apparent. There is a hint of a faint disk, but the spheroid component dominates the overall morphology. Star formation activity appears to be low, based on the lack of significant blue color indicative of young, hot stars. The angular size is relatively compact.
