The galaxy presents as a relatively smooth, disk-like structure, appearing more elongated than circular. The light distribution suggests a central bulge region that dominates in brightness. The main body is characterized by a generally diffused glow. There is little evidence of strong spiral arm structure or significant dust lanes visible in this image, although there are some suggestions of minor disturbances, possibly related to interactions or internal dynamics. There appears to be some merging activity, as the light in the disk seems to be distorted. The galaxy exhibits color gradients, with a slightly redder hue at the central bulge transitioning to a bluer tint in the outer regions of the disk.
