The galaxy appears as a relatively smooth, elliptical object, exhibiting a concentrated central bulge that gradually fades into a more diffuse halo. Its shape is slightly elongated, but predominantly rounded. The color profile suggests a population of older stars, indicated by the reddish-yellow hue. There is minimal evidence of spiral arm structure or significant dust lanes within the galaxy. No signs of on-going major mergers or tidal disturbances are apparent, although some minor irregularities are present on the outskirts of the galactic disc. The galaxy’s overall morphology aligns with that of a typical early-type galaxy with low recent star formation activity.
