The galaxy presents a largely smooth and rounded morphology, with a concentration of light toward the center. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears primarily spheroidal in shape, with the longer side being less than twice that of the shorter. Some minor asymmetry is present, but there's no evidence of tidal tails, or other signs of ongoing major merger activity. There is some indication of disturbances in the outer regions, so minor interaction with neighboring objects is possible. Based on the bluer color toward the center, some ongoing star formation is possible, but not pervasive. The galaxy is likely a relatively massive system, with no sign of any active galactic nuclei.