The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange. There is a subtle fading of color toward the outer regions of the galaxy, suggesting a change in stellar population distribution, with potentially older stars in the central bulge and a relatively younger population in the disk. The overall shape appears mostly round, with perhaps a slight deviation towards a cigar shape. There is no obvious evidence of spiral arm structure or strong dust lanes. There is no noticeable tidal disturbance or other features to indicate an ongoing or recent merger event.
