This galaxy exhibits a complex morphology, suggestive of an ongoing or recent interaction. There are two distinct central concentrations of light. The brighter of these two appears to be a more compact nucleus. These features indicate either a binary galaxy system or a single galaxy undergoing a major merger event. 

The overall color of the object is indicative of a mix of stellar populations. The central regions exhibit a yellowish hue, implying the presence of older stars. The outer regions show a bluer tint suggesting younger, hotter stars, and possibly ongoing star formation.

Faint tidal features appear to be present in the form of streams or tails emanating from the main body of the galaxy, lending further support to the interaction scenario. These features are diffuse and low in surface brightness. There is no prominent spiral structure visible. The object appears somewhat disturbed, lacking a clear disk structure.