The galaxy presents as a relatively compact structure. It exhibits a morphology that appears to be transitioning. There are hints of spiral arm structures, though they are not well-defined, appearing somewhat flocculent. There appears to be a relatively smooth central bulge. The color profile suggests the presence of both older stellar populations, indicated by redder hues, and pockets of active star formation, revealed by bluer regions particularly along the partial spiral arm segments. There is some indication of a tidal tail or possible merger event occuring. There appears to be some dust obscuration along certain regions. The overall shape is not perfectly circular but rather slightly elongated, possibly indicating ongoing interactions or internal dynamics that are still shaping the galaxy.
