The galaxy presents as a relatively compact, elliptical-like system. It exhibits a smooth, diffuse morphology with no apparent spiral arm structure or prominent dust lanes. The core region appears to be centrally concentrated, displaying a bright, yellowish hue which could indicate an older stellar population. The outer regions of the galaxy gradually fade into the background sky, showing a slightly more diffuse and less luminous profile. There is little evidence of ongoing major merger activity, tidal tails or significant morphological disturbance. The overall shape is consistent with an oblate spheroid viewed at an unknown inclination angle.
