The galaxy appears to be a spiral galaxy, viewed at a slight angle relative to edge-on. There is a clear disk structure visible, and evidence of spiral arms. The central bulge is moderately sized, and appears relatively bright. The spiral arms are somewhat loosely wound. There is no evidence of a strong bar structure. The overall morphology appears relatively undisturbed; there is no clear sign of a major merger or significant tidal disruption. Star formation is likely ongoing, based on the bluer colors observed in the disk and spiral arms.
