The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a concentrated, bright reddish-orange core, likely indicative of an older stellar population. A gradual decrease in surface brightness is observed moving outward from the core. The outer regions appear more greenish, possibly suggesting younger, hotter stars or regions of ionized gas. There is no evidence of distinct spiral arms, bars, or other significant structural features such as tidal tails or merging companions. The galaxy's shape is elongated, showing some degree of ellipticity, appearing somewhat cigar-shaped. No major disturbances or mergers are apparent in this image, although there may be a minor asymmetry on the outskirts.
