This galaxy appears to be a relatively luminous spiral galaxy, characterized by a central bulge region and a disk-like structure. The bulge exhibits a yellowish hue, potentially indicating an older stellar population, while the outer regions of the disk display a bluer tint, suggestive of ongoing or recent star formation activity. The disk appears to be more amorphous and lacking well-defined spiral arm structures. There is some evidence of a slight disturbance in the morphology, possibly indicating a past or ongoing minor interaction with another galaxy or a merger event. The galaxy is somewhat smooth in appearance, indicating it is not experiencing a major disruption, but does contain features. It is somewhat elliptical in shape. The disk is relatively compact. There is a slight asymmetry in the distribution of light.
