The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, characterized by a yellowish-orange hue, suggestive of an older stellar population. The outer regions of the galaxy appear less defined, with a gradual decrease in luminosity outwards. There is a slight elongation to the structure, with the galaxy appearing somewhat cigar-shaped rather than perfectly spherical. Possible minor disturbances or asymmetries are observed in the outer regions of the disk. The object appears to be an early-type galaxy with little or no active star formation.
