The galaxy presents as a relatively smooth, elliptical morphology. Its shape appears elongated or cigar-shaped rather than perfectly spherical, suggesting a potential classification as an E4-E7 elliptical. The central region exhibits a high surface brightness, indicating a concentrated stellar population likely composed of older stars. There's a color gradient from the center outwards, with the central bulge appearing yellower than the outer regions, which are bluer. This suggests ongoing star formation, albeit at a low rate, within the outer disk, with the bluer light indicating the presence of younger, hotter stars. There does not appear to be any major disturbances in the galaxy.
