This galaxy appears to be a relatively smooth, disk-like structure viewed at an angle. The central bulge exhibits a concentrated, bright yellowish-orange hue, suggesting a population of older stars. The disk component is faint and the outer edge is a more greenish yellow, potentially indicative of some ongoing star formation, although at a low rate. The disk is elongated, appearing somewhere between round and cigar-shaped. There is a subtle hint of disturbance or asymmetry in the outer regions, but no clear evidence of major mergers or tidal features is immediately apparent. The galaxy appears relatively isolated.
