The galaxy presents a primarily smooth morphology, suggestive of an elliptical or lenticular type. It exhibits a concentrated central bulge with a yellow-gold hue, likely indicating an older stellar population. The outer regions of the galaxy appear less concentrated and fainter, with a subtly bluer color. The overall shape is moderately elliptical, appearing to be somewhere between a perfect circle and a cigar shape. There is no discernible spiral arm structure or strong evidence of recent major mergers or significant tidal disturbances. The smoothness of the light distribution and the central concentration suggest minimal ongoing star formation within the galaxy.
