The galaxy presents as a centrally concentrated elliptical or lenticular system. Its morphology is largely smooth and features an oblate spheroidal shape that is slightly round. The light distribution reveals a prominent bulge, indicated by the concentration of yellowish light toward the center. Some evidence of low level star formation is present. There is no clear presence of an actively merging system, major disturbances, tidal tails, or other clear irregularities. The galaxy exhibits a notable color gradient. The core region radiates with a yellow tone, transitioning to a redder hue towards the outer regions. The overall structure is generally undisturbed, which would imply it is relatively quiescent.
