The galaxy presents as a relatively compact, centrally concentrated object. The core exhibits a smooth, diffuse light profile. The outer regions fade gradually, maintaining a mostly elliptical or circular symmetry. There are no obvious spiral arms, bars, or distinct dust lanes visible. The color is consistent throughout, exhibiting an emission primarily in the green wavelengths. There is no apparent evidence of strong tidal features or major disturbances, though some subtle irregularities in the outer light distribution cannot be entirely ruled out given the image quality. The overall morphology suggests an early-type galaxy, potentially an elliptical or lenticular galaxy.