The observed galaxy presents as a relatively compact object with a centrally concentrated, bright core. Based on color gradients, the inner region appears to be dominated by bluer wavelengths, transitioning to a more reddish hue in the outer regions. The morphology is primarily smooth, with a possible very subtle disturbed feature visible. The main body appears largely spheroidal with little indication of a developed disk structure, although there are vague arm-like structures hinting it could be a spiral galaxy or disk galaxy of some kind. Overall the galaxy seems relatively isolated.
