The galaxy presents as a somewhat diffuse object with an elliptical morphology. The light is primarily concentrated toward the center, exhibiting a smooth profile with a gentle falloff in intensity towards the edges. The core region does not appear to have a highly concentrated or point-like nucleus. There is a slight hint of a disk-like structure but it is not clearly defined, perhaps due to its inclination or inherent properties of the galaxy itself. There doesn't appear to be any current major merger activity. The redder color suggests an older stellar population and/or dust obscuration.
