The galaxy exhibits a morphology dominated by a smooth, elliptical-like structure. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in surface brightness extending outwards. The overall shape appears to be somewhat elongated, possibly indicating an intermediate classification between a perfectly round and cigar-shaped elliptical galaxy. There appears to be a distinct and concentrated region of star formation. The galaxy does not appear to be undergoing any major merging events.
