The galaxy presents a generally smooth, elliptical morphology. It appears moderately elongated, exhibiting a cigar-like shape. The central region shows a high concentration of luminosity, likely indicative of a galactic bulge. There is a subtle color gradient, with the core region appearing more yellow, which could be due to a population of older, redder stars. The outer regions are less well-defined, fading into the background sky. No distinct spiral arm structures or significant dust lanes are apparent in this image. There is no evidence of major mergers or tidal disturbances. Minor disturbances, if present, would be difficult to resolve at this image quality.
