The galaxy appears to be a spiral galaxy, exhibiting a clear disk structure. Prominent spiral arms extend from the central bulge. The arms seem tightly wound around the bulge. The central bulge appears moderately sized, emitting a relatively consistent light profile. Dust lanes may be present within the spiral arms, but this is difficult to confirm due to the image resolution. No signs of a strong bar structure are visible. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances, maintaining a relatively undisturbed morphology.
