The galaxy presents as an elongated, cigar-shaped system. It exhibits a relatively smooth, centrally concentrated light distribution with no immediately apparent spiral arm structures or prominent star-forming regions. The core appears as a diffuse yellowish glow, suggesting a population of older stars. The outer regions show a bluer hue, indicative of a younger stellar population. There is a subtle transition in color and brightness from the central bulge to the outer disk. The overall symmetry indicates a lack of recent major merger events, although a minor disturbance cannot be ruled out based solely on this image. The morphology suggests a relatively evolved system, possibly a lenticular galaxy or an edge-on spiral galaxy.
