The galaxy presents as a moderately bright, elliptical structure with a smooth, diffuse appearance. A dominant, concentrated central bulge exhibits a yellowish-orange hue, suggesting an older stellar population. The overall form of the galaxy is somewhat rounded, though not perfectly spherical, possibly closer to in between round and cigar shaped. Subtle disturbances appear present, though not prominently. There may be evidence of a minor interaction or past merger event. Star formation rates appear suppressed.
