The galaxy presents as a slightly elongated, lenticular structure with a prominent central bulge. The galaxy exhibits a relatively smooth appearance overall, although there are subtle hints of an extended disk. The light distribution indicates a concentrated central region that likely hosts older stellar populations. There appears to be a disk, which may be host to some minor star formation. Given the smoothness of the galaxy and the dominance of the bulge, it is likely an evolved system that is in the process of winding down its star formation activity. There appears to be a neighboring galaxy nearby, which may or may not be related to the structure of the galaxy being analyzed.
