The galaxy presents a disturbed morphology, suggestive of ongoing or recent gravitational interaction. While the primary body of the galaxy appears relatively compact, there are noticeable asymmetries and distortions in its outer regions.

The overall light distribution is not smooth. There appears to be a dominant central concentration of luminosity, possibly indicating a bulge component. The outer regions exhibit a clumpy structure, with several distinct knots of brighter emission distributed across its area. These knots might represent regions of heightened star formation activity, potentially triggered by the interaction. There are also areas of lower surface brightness extending outwards, indicating tidal features. There is a tail extending to the top of the image.

Based on this evidence, the galaxy is likely undergoing a merger. There is not enough evidence in this image to determine if this is a minor or major merger.
