The galaxy presents as a concentrated, yellowish-white elliptical system. It appears predominantly smooth in texture with a centrally concentrated light distribution, suggesting an older stellar population. There is a slight elongation, indicating a non-spherical morphology that leans towards an intermediate shape between round and elongated. There is a subtle hint of disturbance and asymmetry. The galaxy is not obviously undergoing a major merger, but there appears to be a slight distortion in its light distribution, with some suggestion of minor interactions. The color profile reveals a relatively passive system with negligible ongoing star formation, which is consistent with the smooth morphology.
