The galaxy presents as a somewhat amorphous, though generally elliptical, distribution of light. It appears to be in a dynamic state, potentially undergoing some form of interaction or disturbance. A central concentration of yellowish light dominates the core region, suggesting an older stellar population. Fainter, diffuse greenish-blue light extends outward, creating a halo-like structure. There appear to be subtle features, such as asymmetries or irregular patches of color, particularly in the outer regions, which might indicate tidal features or ongoing star formation. Given the irregular features there may be minor merger event occurring. Overall, the galaxy exhibits a moderate level of internal complexity.
