The galaxy presents as a centrally concentrated, roughly elliptical object. The core region exhibits a bright, yellowish-white luminosity suggesting a population of older stars. Fainter bluish light is present throughout the disk, indicative of the presence of younger, bluer stars, and star formation. The outer regions of the galaxy show lower surface brightness, fading into the background sky. There is no strong evidence of spiral arm structure or a well-defined disk. The overall structure suggests a relatively evolved system, possibly with some ongoing, low-level star formation. The galaxy is oriented with its major axis extending horizontally across the image. It appears relatively undisturbed, with no obvious signs of tidal interactions or major mergers, though some minor disturbance is possible. The shape of the galaxy is more round than cigar shaped.
