The galaxy presents a disturbed morphology, suggestive of an ongoing or recent merger event. The main body of the galaxy exhibits a complex structure with luminous regions of yellowish hue, possibly indicating older stellar populations or regions of intense star formation enshrouded in dust. Fainter, diffuse extensions are visible, lending to its asymmetric shape. The galaxy has an estimated size of about 11.5 kpc.

There are hints of tidal features or disrupted arms extending from the primary structure, which are consistent with a galaxy undergoing a merger. The overall color suggests a significant population of evolved stars, however, the presence of regions with relatively blue light implies active star formation is also occurring in some locations within the system. Based on these observations, it can be surmised that the galaxy's star formation rate is moderate, but the event seems to be heavily influenced by the ongoing merger. The estimated log(stellar mass) is high, but still allows for potential interactions.
