The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge that transitions into a diffuse halo. The core region appears to be composed of older stellar populations, indicated by the yellowish hue, suggesting minimal ongoing star formation in the central regions. Fainter outer regions show bluer colors, implying the presence of some younger, hotter stars, or potentially indicating some recent minor merger activity. The galaxy is somewhat elongated in shape, but does not display any pronounced spiral arm structures, ring features, or signs of major tidal disturbances or active galactic nuclei activity. It appears to be a fairly quiescent galaxy.