The galaxy presents as a moderately bright, elliptical-like structure. Its color appears to be redder in nature, indicating an older stellar population. The galaxy exhibits a relatively smooth light distribution with a centrally concentrated bulge and little evidence of spiral arms or dust lanes. There is a slight elongation in the overall shape, suggesting it is not perfectly spherical but somewhat flattened. The overall structure suggests a lack of significant ongoing star formation and the presence of a passively evolving galaxy. There may be a possible minor interaction with a much smaller nearby object.