The galaxy presents as a somewhat elliptical structure with a smooth light distribution. The central region exhibits a significantly brighter and more concentrated luminosity, suggesting a substantial stellar population or possibly an active galactic nucleus. Proceeding outward from the core, the luminosity gradually decreases, showing a relatively smooth transition into the outer regions. The galaxy displays a color gradient, appearing more yellow-reddish in the core, potentially indicating an older stellar population. The outer regions appear slightly bluer, hinting at the presence of some younger, hotter stars, though overall star formation activity seems relatively low. There is no prominent spiral arm structure or obvious signs of major mergers or strong tidal disturbances, with only minor disturbances possible. The galaxy's shape is somewhere in between round and cigar shaped, with a tendency towards being more elongated than fully circular.
