The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that is bright and primarily yellowish-orange in color, suggesting a population of older stars. The main body of the galaxy is elongated, though it appears more 'in between' oval and cigar shaped. The light gradually fades into the surrounding space, indicating a diffuse halo. There are no obvious signs of a spiral structure or significant dust lanes. No major merger events appear to be currently occurring. The overall appearance suggests that this galaxy has undergone significant evolutionary processes and is not currently undergoing high rates of star formation.
