The galaxy exhibits a disturbed morphology, indicating possible interaction or merger activity. A central bulge region shows a yellowish hue, suggestive of an older stellar population. The galaxy presents a somewhat asymmetric shape with fainter blueish regions extending outwards, which imply active star formation. There appears to be a tidal tail or stream extending from one side of the galaxy, further supporting the hypothesis of a recent gravitational interaction. The overall color gradient of the galaxy suggests an active evolution, moving away from a smooth regular morphology.