The galaxy presents a generally smooth, elliptical morphology. The light distribution indicates a high degree of central concentration, appearing almost spheroidal. There is a subtle color gradient, transitioning from a bluer hue in the core region to redder tones in the outer edges. Faint, diffuse extensions are present, lacking a distinct disk-like structure. Overall, the morphology is suggestive of a galaxy that has largely exhausted its gas reservoir, and is now composed predominantly of older stars. Evidence of recent or ongoing major mergers appears to be absent; however, a subtle asymmetry might indicate a minor interaction in its past. Star formation is likely low.
