The galaxy presents as a relatively smooth and centrally concentrated object. The light profile appears diffuse, lacking a strong spiral arm structure or a prominent bar. The overall shape is approximately round, with a slight elongation. Color gradients are subtle, showing a generally redder core transitioning to slightly bluer outer regions. This suggests the presence of older stellar populations in the central regions and possibly younger stars at the outskirts. There is little evidence of significant recent mergers or major tidal disturbances in this image.
