The galaxy appears to be a spiral type, exhibiting a prominent disk structure. Two distinct spiral arms are visible, demonstrating a moderate to loose winding pattern as they extend from the central bulge. The bulge itself is relatively moderate in size, contributing a significant portion to the overall luminosity of the galaxy's core.

There is a subtle suggestion of a bar structure within the central region, although it does not appear particularly pronounced. The galaxy's color gradient suggests active star formation, indicated by bluer hues concentrated in the spiral arms, contrasting with the yellower tones of older stellar populations in the bulge. The disk of the galaxy is oriented somewhat face-on, allowing for a clear view of its spiral structure. The overall morphology suggests a relatively undisturbed system, with no apparent signs of a recent major merger event. There are possibly signs of a minor disturbance in the galaxy's shape, such as asymmetries in the spiral arm structure.
