The galaxy presents as a somewhat amorphous, elliptical-like structure. It exhibits a smooth overall appearance, with a subtle color gradient that suggests a concentration of older stellar populations towards the central region. The core appears slightly reddish, transitioning to a bluer hue in the outer regions. The isophotes are moderately elongated. There is no obvious evidence of spiral arm structure, prominent dust lanes, or a distinct central bulge. The galaxy does not seem to show strong signs of ongoing major mergers or significant tidal disturbances.
