The galaxy presents as a centrally concentrated object. There is a bright, unresolved core suggesting the presence of either a dense stellar population or an active galactic nucleus. Surrounding the core is a diffuse, elliptical halo, which transitions smoothly outward, with no distinct boundary. The light distribution within the halo is somewhat uneven. There are subtle indications of faint spiral arm structures embedded within the broader halo, though these features are not sharply defined. The overall color profile appears relatively uniform, with a slightly bluer hue in the outer regions, possibly indicative of younger stellar populations. A faint, asymmetric extension can be observed on one side, suggesting a potential tidal interaction or minor disturbance. No prominent dust lanes are visible, and the galaxy does not exhibit a highly flattened disk.
