The galaxy presents as a single, relatively smooth, centrally concentrated object. It exhibits a dominant, spheroidal bulge component that is yellowish-white. The lack of visible spiral arms or distinct dust lanes suggests a classification towards the elliptical or lenticular end of the Hubble sequence, potentially an E or S0 galaxy. The object is slightly elongated. There are no clear signs of major tidal disturbances or active galactic nuclei jets emanating from the core. Faint diffuse halo surrounds the central, brighter region. The color indices suggest the stellar population is dominated by older stars. There appears to be a smaller, fainter component offset from the main object, which could be a minor merger or tidal debris.
