The galaxy presents as a merging system, possibly in the late stages of interaction. The primary body exhibits a somewhat irregular, elongated morphology, lacking a well-defined spiral structure or elliptical shape. A secondary, smaller component is visible and appears to be significantly gravitationally distorted, its light distribution suggestive of tidal disruption.

The color profile indicates a primarily older stellar population, exhibiting a yellowish hue concentrated toward the central regions of both components, this hints at a relatively low rate of current star formation. There are bluer regions visible in what might have been the outskirts of each system, possibly signifying areas of ongoing but weak star formation. The system's light is moderately concentrated. The overall appearance suggests a considerable mass, though the activity level appears to be relatively low. There is evidence of dust lanes or uneven distributions, particularly along the edges of the main body. Overall, it suggests two systems of significant mass that are in the late stages of merging with little major ongoing starbursting.