The galaxy presents as a roughly elliptical structure with a smooth, diffuse light distribution. The central region exhibits a higher surface brightness, appearing as a concentrated bulge of light that is slightly bluer than the outer regions. Faint, diffuse extensions surround the main body of the galaxy, suggesting a possible extended halo or tidal features, though no clear spiral arm structure or pronounced dust lanes are visible. The lack of distinct features and the smooth light profile indicate it may be an early-type galaxy, likely an elliptical or lenticular. There's a subtle color gradient, shifting from slightly bluer in the core to redder in the outer regions, potentially indicating differing stellar populations or dust content across the galaxy. No apparent signs of ongoing major mergers are detected, but minor disturbances might be possible.
