The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a bright, concentrated luminosity, suggestive of a high stellar density or a possible active galactic nucleus, although not directly visible in this image. The overall shape is neither perfectly spherical nor significantly elongated, appearing somewhat in-between with a slight cigar shape. There is a subtle hint of a disk-like structure with a small ring that is slightly off center, but the dominant characteristic is its smooth, diffuse halo. The color profile shows a slight reddening toward the core, potentially indicative of an older stellar population in the central regions. Based on its morphology, this galaxy could have recently underwent a minor disturbance or is in a state of quiescence, with limited ongoing major star formation activity.
