The galaxy presents as a centrally concentrated, elliptical morphology. The core region exhibits a bright, diffuse glow that is most likely comprised of older stars, as evidenced by the reddish-yellow hue. There is minimal observable structure, such as spiral arms or distinct dust lanes, suggesting a relatively smooth stellar distribution. The galaxy’s overall shape appears quite round. The outer regions of the galaxy fade gradually into the background, indicating a lack of sharp edges or distinct boundaries. There does not appear to be evidence of any major ongoing merging activity or significant tidal disturbances. The color profile and smooth morphology suggest this is an early-type galaxy with little active star formation.
