Observed galaxy presents as a compact, seemingly elliptical structure with a noticeable, bright central concentration. The core region appears to be relatively smooth with an intense emission. The outer regions exhibit a more diffuse character. There appears to be slight asymmetry in the outer halo, specifically some patchy red coloration. The galaxy does not appear to show any obvious spiral arm structure or distinct disk. There may be very minor distortions in the outer halo suggesting a possible past merger event. It is also possible these could be related to data processing issues.
