The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a bright, yellowish-white luminosity, indicative of an older stellar population. Moving outward from the core, the light becomes more diffuse, with a faint blue tinge in its halo region, suggesting the possibility of some younger stars present.

There is no evidence of well-defined spiral arms or a distinct disk structure; the light distribution is relatively smooth and spheroidal. The isophotes appear largely regular, but subtle irregularities could indicate minor disturbances or interactions in its recent past. There does not seem to be any current major merger activity apparent based on the image. The overall color suggests a transition region object.
