The galaxy presents as a spiral type, exhibiting a notable disk structure viewed at an angle oblique to edge-on. Prominent spiral arms are observed, displaying a tightly wound morphology with a high degree of symmetry. The central bulge is readily apparent, possessing a moderate relative size in comparison to the overall galactic disk, appearing very bright and concentrated. A prominent bar is also visibly intersecting the central bulge. Star formation appears present within the arms. There are no signs of major ongoing mergers, however there is some irregularity that suggests possible minor disturbances or interactions. The galaxy appears largely isolated.
