The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. The core exhibits a yellowish-orange hue, indicative of an older stellar population. The outer regions display a gradual decrease in surface brightness, with some bluer tones emerging. There may be a faint, diffuse disk component. The overall shape is elongated, but it appears to be closer to round than cigar-shaped. There is no clear evidence of major mergers or tidal disturbances. The features suggest that star formation is present but at a low rate.
