The galaxy presents as a relatively compact object, approximately elliptical in shape, with a primary axis maybe twice as long as the minor axis. The light profile appears centrally concentrated with a smooth, gradual decline in surface brightness outwards. The primary color is a muted bluish-white, with a hint of red in the upper left and right portion of the galaxy. This suggests a mix of stellar populations, potentially with older, redder stars concentrated in the core, and the presence of recent or ongoing star formation. There is no clear evidence of spiral arm structure, prominent dust lanes, or other features commonly associated with disk galaxies. Overall, the morphology suggests a relatively evolved system. There may be a slight disturbance within the galaxy suggesting a potential minor merger event in its past, but this is hard to confirm.
