The galaxy presents a morphology characterized by a relatively smooth, elliptical-like structure. A slight elongation is observed, but it appears generally rounded. The central region exhibits a bright concentration of light, likely indicating a dense nucleus. The outer regions gradually fade, displaying a diffuse halo surrounding the core. There's a subtle color gradient from the center outwards, potentially suggesting differential stellar populations or dust distribution. A very slight disk-like structure may be present. No signs of major mergers or tidal disturbances are readily apparent, although some possible minor asymmetries or disturbances may be present, indicating minor interactions. The overall color profile suggests ongoing star formation, but relatively low rates. The estimated physical size indicates that this is an intermediate-sized galaxy.
