The galaxy presents as a smooth, cigar-shaped elliptical. Its light distribution appears concentrated towards the center, with a gradual fading towards the elongated edges. The primary color of the galaxy is a yellowish-orange hue, suggesting an older stellar population with a lower rate of on-going star formation. There is no visible evidence of spiral arm structure or significant dust lanes. No signs of a recent or ongoing major merger event are visible. The overall morphology suggests a relaxed system that has likely undergone significant dynamical evolution.
