The galaxy presents a roughly circular morphology with a bright, concentrated central region. The light distribution appears relatively smooth, suggesting a possible elliptical or lenticular classification, although the possibility of a face-on spiral galaxy with a dominant bulge cannot be excluded. There's a slight elongation of the central brightness concentration, hinting at some level of internal structure or asymmetry. The color gradient exhibits a subtle variation, with a bluer hue concentrated towards the central region and a slightly redder periphery. There's also the possibility of a merger or tidal disturbance.
