The galaxy presents as a relatively smooth, elliptical structure. Its light is concentrated towards the center, exhibiting a bright, yellowish-orange core that gradually fades into the outer regions. The galaxy's shape is elongated, with a cigar-like appearance rather than a perfect sphere. A subtle disk-like structure with hints of spiral arms seems to be present, but is not well defined. No strong indications of major disturbances or ongoing mergers are apparent, though a slight asymmetry may suggest a minor interaction or internal perturbation. The overall color suggests a population of older stars, though some blueish-green tints in the outer regions suggest a small level of on-going star formation.
