The galaxy presents as a somewhat flattened, disk-like structure, viewed at a significant inclination. The central region appears significantly brighter and more concentrated, exhibiting a nearly unresolved, compact nucleus. Proceeding outward from the core, a subtle color gradient is detectable; the inner region displays a greenish hue, transitioning to a more blueish tint in the extended halo surrounding it. A faint, more yellowish ring appears to surround this inner core and could either be a ring formation or caused by the inclination of the disk itself.

There is the hint of a faint plume or extension on one side, which could be evidence of a possible minor merger or tidal interaction, suggesting gravitational disturbance, however, this is subtle. The overall smoothness of the galaxy indicates the likelihood of an elliptical or lenticular type, although the possible outer extension may suggest a disturbed disk structure. There may be a merger event occurring.
