The galaxy presents as a primarily smooth object, with a distinct central bulge region. The overall shape is somewhere in between round and cigar-shaped, with a slight elongation visible along what appears to be a major axis. Hints of a disk-like structure are seen, although any spiral arm features are not readily apparent. There appears to be little to no significant ongoing merging activity or major disturbances to the galaxy's structure. The colors of the galaxy suggest the presence of both older stellar populations in the central bulge, as well as the possible presence of some younger, bluer stars within the disk. The galaxy appears to be a relatively massive galaxy, likely with suppressed star formation activity.
