The galaxy presents as a relatively smooth and rounded object, displaying a prominent central bulge that appears bright and concentrated. There is a subtle color gradient from the center outwards, suggestive of differing stellar populations, with the core potentially housing older, redder stars. The galaxy appears to be largely devoid of significant spiral arm structures or dust lanes, lending to its overall smooth appearance. There are hints of faint, diffuse outer regions extending from the main body, indicating the presence of a halo or extended stellar distribution, though the resolution makes detailed analysis challenging. No obvious signs of a major ongoing merger or significant tidal disturbances are readily apparent.
