The galaxy presents as a centrally concentrated spheroid with a relatively smooth light distribution. There is no apparent spiral arm structure or bar. The morphology suggests a largely featureless elliptical galaxy or potentially a lenticular galaxy viewed face-on. The core exhibits a yellowish hue, possibly indicating an older stellar population. The outer regions are less luminous and appear slightly bluer in comparison, which could signify the presence of a younger stellar population relative to the core but not significant enough to disrupt the overall smoothness. Based on these qualities, the galaxy appears to be relatively evolved with minimal ongoing star formation.
