The galaxy presents as a spiral structure with a moderate-sized bulge. The spiral arms appear relatively tightly wound in some areas. The dominant color is bluish, suggesting ongoing star formation in the spiral arms, with some regions of redder hues, possibly indicative of older stellar populations. The galaxy is neither perfectly face-on nor edge-on, allowing for a clear view of its spiral structure. There is no apparent strong bar structure, but there may be a weak bar. The spiral arms are well-defined, extending outwards from the central bulge. There may be some minor disturbances evident within the spiral arms, potentially indicating interactions or past mergers.
