This galaxy exhibits a complex morphology indicative of a potential merger event. It presents as a centrally concentrated object with what appears to be two distinct, bright nuclei separated by a relatively short distance. These nuclei display a yellowish-white color, suggesting older stellar populations or significant dust obscuration. Faint extensions surround the primary body of the galaxy, possibly tidal tails or disrupted spiral arms, a common feature in interacting systems. There is a slightly elongated structure, but lacks a defined spiral or elliptical shape, indicating a disturbed morphology. The overall color profile leans towards redder wavelengths, implying relatively low recent star formation activity.
