The galaxy presents as a spiral type, characterized by a well-defined disk structure. A prominent central bulge is visible, appearing moderately sized relative to the disk. Evidence suggests the presence of a bar structure within the bulge region, with an intensity ranging from weak to strong.

The spiral arms exhibit a grand design, tightly wound in some regions, with medium winding in others, and loosely wound arms visible as well. The galaxy exhibits a primarily two-armed spiral morphology.

The overall color profile suggests active star formation occurring within the disk, as indicated by a relatively bluer hue in the spiral arms when compared to the central bulge. There is no significant morphological evidence for ongoing major mergers or significant tidal disturbances, although minor disturbances cannot be ruled out.
