The galaxy presents an elongated, possibly disrupted morphology, spanning an estimated 7.5 kpc in effective radius. A bright, concentrated central region of intense red color is evident, suggesting a concentration of older stellar populations and/or significant dust obscuration. Extending outwards from this central region is a fainter, blue-tinged structure which appears to be a tidal tail feature, likely resulting from gravitational interaction. This feature indicates ongoing or recent interactions with another galaxy. The galaxy exhibits evidence of active star formation in its extremities, as suggested by its blue color. The overall appearance suggests a system undergoing a merger or experiencing strong tidal effects, contributing to the disturbed morphology and localized star-forming regions.
