This galaxy appears to be a relatively bright, well-defined object. Its morphology suggests it is primarily smooth, though not perfectly spherical. It presents an elliptical shape, appearing more elongated than circular, but not extremely cigar-shaped. There is evidence of a disk-like structure but it is very weak, which could be an indication of ongoing star formation. No strong signs of a major merger event are apparent, though there may be some minor gravitational disturbance in its morphology. Overall, it appears to be an intermediate mass galaxy, with a moderate star formation rate, and its color suggests it is at a redshift distance.
