The galaxy presents as an irregular, somewhat diffuse structure. Its overall color appears to be reddish, suggesting a population of older stars and/or significant dust obscuration. No distinct spiral arms or a well-defined central bulge are readily apparent. There is a subtle elongation or asymmetry to the overall shape, but not obviously disk like. Possible faint tidal features or minor disturbances are hinted at within the galaxy's morphology. The appearance leans towards a merging event. Based on its overall structure, the galaxy is likely undergoing some level of interaction or disturbance. 
