The galaxy presents a generally smooth, rounded appearance, with a centrally concentrated bulge exhibiting a high degree of luminosity. There is a suggestion of disk-like structure emanating from the central bulge, however it appears to be highly disturbed, perhaps tidally disrupted, or as a result of a recent merger event. There is visible evidence of ongoing star formation, especially in the extended arm or tail extending from the galaxy, as indicated by a bluer colour, however, this may also be dust. It appears to be undergoing a major interaction with another galaxy or is in the late stages of a merger, showing a strong disturbance in its morphology.
