The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, centrally concentrated light profile, suggesting a dominant spheroidal component. The core region displays a yellow-white hue, potentially indicative of an older stellar population. Fainter, bluer outskirts hint at the presence of some younger stars, possibly within a flattened disk component, however this is less pronounced. There are hints of a minor disturbance or interaction, visible as a slight asymmetry in the outer regions.
