The galaxy exhibits a complex morphology, appearing as a system potentially undergoing a merging event. Two distinct, bright components are observed, suggesting the presence of two galactic nuclei or concentrations of stellar material. The dominant color is yellowish, which could indicate an older stellar population. The overall shape is relatively smooth, but is noticeably disturbed. A slight hint of a possible tidal tail feature, although indistinct, extends away from the main body, further supporting the hypothesis of an ongoing or recent merger. The size of the galaxy appears moderate.
