The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular type. The central region exhibits a high concentration of light, appearing bright and nearly spherical. There is a subtle color gradient, with the core trending towards a yellowish-white hue, potentially indicating an older stellar population. Surrounding the central bulge, a faint, diffuse halo is observed, lacking distinct structural features such as spiral arms. This halo fades gradually into the background sky. There are some faint hints of disturbance that may or may not be associated with tidal interactions. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
