The galaxy exhibits an irregular morphology, potentially indicative of an ongoing or recent interaction. It appears to be composed of two distinct luminosity concentrations, a brighter, more compact, blue-hued region and a less concentrated, elongated, yellow-toned region. The blue region may suggest a population of younger, hotter stars undergoing active star formation. The yellow region shows a smoother texture, hinting towards an older stellar population. There appears to be an additional clump of light to the left of the main structure, as well as a faint extension stretching from the central region. There is evidence of possible tidal features, particularly a faint extension, further indicating gravitational interactions. The overall structure deviates significantly from a typical spiral or elliptical morphology.
