The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular classification. It exhibits a centrally concentrated brightness profile with a smooth falloff of luminosity towards its outer edges. The core region appears yellowish-white, which is consistent with an older stellar population. The galaxy's overall shape is neither perfectly spherical nor highly elongated, but rather shows a moderate ellipticity. Faint, somewhat indistinct structure may indicate a possible disk or some faint spiral arms. There are hints of minor disturbances, but no clear signs of an active merger event. The galaxy's colors indicate it is a relatively massive galaxy with a relatively low rate of ongoing star formation.
