The galaxy presents as a single, largely smooth, unresolved object at a redshift of approximately 0.1. The morphology suggests a dominant spheroidal component. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. There is a slight color gradient, with the central region appearing somewhat bluer than the surrounding halo, suggesting a possible concentration of younger stars towards the core. There is no visual evidence of spiral arms, bar structures, or significant dust lanes. There are no clear signs of interaction or major mergers. A faint, diffuse halo surrounds the central concentration, fading into the background sky.
