The galaxy presents an elliptical morphology, appearing cigar-shaped with a noticeable elongation. Its central bulge is bright and concentrated, displaying a yellowish-white hue, which suggests a population of older stars. The outer regions show a gradual fading in luminosity. There may be a disk component visible in some of the outer areas, potentially containing areas of on-going star formation. The galaxy appears to be relatively undisturbed, showing no signs of a major merger event and only minor irregularities. The overall color profile indicates a relatively low rate of star formation.
