The galaxy presents a generally smooth appearance, though some features suggest the presence of a disk structure. It appears to be elliptical in shape, although not perfectly round; it leans towards being 'in between' round and cigar shaped. The central region is visibly brighter and more condensed. There is possible minor disturbances and/or minor merging as well. The color profile indicates a redder tint on the outskirts, hinting at older stellar populations there. The central area is bluer, suggesting some active or recent star formation, although potentially not at a high rate.
