The galaxy presents as a spiral type, viewed at an oblique angle. The disk is prominent, exhibiting a defined structure with discernible spiral arms. These arms appear tightly wound and display a predominantly blue hue, suggestive of ongoing star formation. A central bulge is visible, characterized by a yellowish color, indicating a population of older stars. The galaxy shows no obvious signs of a significant bar structure. The morphology suggests the galaxy is relatively undisturbed, with no apparent major merger events in its recent history. However, there is possible minor disturbance.
