The galaxy presents as a centrally concentrated, elliptical system. A smooth, diffused halo surrounds a brighter, more compact core. The color profile suggests a redder core transitioning to a bluer halo. The presence of a disk is unclear, but possible, and the color change could be explained by an older stellar population in the core, with ongoing star formation in the surrounding regions. There appears to be no evidence of ongoing major merger activity, but perhaps minor disturbance.
