The galaxy presents as a slightly inclined, elongated disk. The central bulge is subtly pronounced and exhibits a yellowish-white hue, suggesting a population of older stars. Proceeding outwards from the bulge, the disk shows a blend of colors with hints of bluer regions, indicating the presence of younger, hotter stars and possibly ongoing star formation. The galaxy does not appear to have prominent spiral arm structures. The edges of the disk appear somewhat diffuse rather than sharply defined. No major merger events or strong tidal disturbances are apparent, but there may be a minor disturbance along one edge. Overall, the galaxy seems to be relatively undisturbed and exhibits characteristics of a late-type spiral or lenticular galaxy.
