The galaxy presents as a primarily smooth object with a generally elliptical morphology. The light distribution appears concentrated toward the center, suggesting a prominent bulge. There may be some minor disturbances or irregularities present, but they do not appear significant enough to classify the galaxy as undergoing a major merger. The color profile indicates a reddish hue, potentially indicating an older stellar population or significant dust obscuration. The overall appearance is consistent with that of an early-type galaxy, perhaps an elliptical or S0. The galaxy appears to be neither perfectly round nor highly elongated.
