The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is noticeably flattened, exhibiting an apparent axial ratio of approximately 0.8. A distinct central bulge is observed, characterized by a bright, concentrated luminosity profile indicative of a high stellar density. There is some disk present. The galaxy's light distribution appears symmetrical, with no obvious signs of major tidal disturbances or ongoing mergers. The color gradient suggests a relatively old stellar population, with a redder hue dominating the central regions and becoming slightly bluer toward the outer regions.
