The galaxy presents as a slightly elongated, centrally concentrated system. The core region exhibits a yellowish-white hue, suggesting a population of older stars. Moving outwards, the light gradually fades. There is a subtle hint of spiral structure, but it appears highly flocculent and disrupted, with a very slight blue tint. The overall form suggests a galaxy that may be undergoing, or has undergone, a merging event. There is no indication of a strong central bar or any dominant spiral arms. The galaxy presents a fairly smooth light profile, though not perfectly uniform.
