The galaxy presents as a single, relatively smooth object with a slightly elongated shape. The light distribution appears concentrated, suggesting a morphology tending towards elliptical. The object's color profile exhibits a general yellowish-red hue, possibly indicating an older stellar population with lower ongoing star formation, as the blue light is more subdued. Irregularity in shape points towards a potential minor interaction or internal disturbance. Given the size and estimated distance, this galaxy is a relatively massive system. It seems to be an elliptical galaxy, possibly undergoing a minor merger.
