This galaxy appears to be a spiral galaxy viewed at a moderate angle, not quite face-on but not edge-on either. The spiral arms are distinct and relatively tightly wound. The central bulge is moderately sized, exhibiting a yellowish hue which may indicate a population of older stars. The arms themselves display bluer regions, potentially regions of active star formation. There is evidence of a bar-like structure. There are some visual disturbances and asymmetry, possibly caused by tidal interactions or ongoing mergers. The overall color suggests a galaxy with ongoing star formation and a significant population of older stars.
