The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and concentrated light distribution. The morphology suggests a relatively evolved system. The core region displays a yellowish-orange hue, potentially indicating an older stellar population or significant dust obscuration. The outer regions transition to a more diffuse, greenish-yellow color. The isophotes appear mostly regular and elliptical, with no obvious signs of strong tidal interactions or major mergers. There may be a slight elongation in one direction, suggesting a mild departure from perfect ellipticity, but overall, the galaxy seems fairly relaxed and undisturbed. There is evidence of some star formation, though likely at a low rate. The estimated size of the galaxy is approximately 5.5 kpc in radius.
