The galaxy presents a predominantly smooth morphology, with a bright, concentrated central bulge. The object exhibits a somewhat elliptical shape, appearing more rounded than elongated. A faint, diffuse disk is visible extending outward from the bulge, although its structure is not well-defined. There are no apparent signs of strong tidal interactions or major mergers; however, a slight asymmetry in the outer regions might indicate a minor disturbance. The galaxy's color profile suggests an older stellar population, based on its reddish-yellow hue.
