The galaxy appears to be a relatively bright, moderately sized, and slightly asymmetric system. There is evidence of a possible ongoing interaction, or recent merger event. The primary body presents a smooth, centrally concentrated morphology. A secondary component is observed to the west, potentially representing a smaller galaxy interacting with the primary system. This secondary component exhibits a bluer hue compared to the primary, suggesting a population of younger, hotter stars. Overall the system could be in the process of merging, the primary body may be a former elliptical galaxy that has recently begun interacting with a nearby dwarf galaxy. 
