This galaxy presents as a lenticular-like form, with a smooth, elliptical light distribution indicative of a significant spheroidal component. The primary color gradient shifts subtly from a light blue to a redder hue towards the outer edges, hinting at possible variations in stellar populations or dust content. The lack of defined spiral arms or distinct features suggests a relatively quiescent state, possibly an early-type galaxy with reduced star formation. Subtle perturbations could indicate minor gravitational interaction with smaller objects, or the galaxy might be an intermediate disk that will one day become a red and dead galaxy.
