The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a noticeable lack of prominent spiral arms or disk-like features. The light distribution appears generally uniform and decreases smoothly from the center outwards. The core exhibits a bright, yellowish hue, potentially indicative of an older stellar population. The galaxy is roughly elliptical in shape, appearing more 'in between' round and cigar-shaped than either extreme. There is no visual evidence of ongoing mergers, major disturbances, or tidal tails. Based on its appearance, this galaxy appears to be a mature system, potentially exhibiting very low levels of star formation.
