The galaxy presents as an elongated, disk-like structure, seen at a significant angle relative to our line of sight. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. Moving outward from the bulge, a flattened disk is visible. The disk shows some evidence of structure, but not tightly wound spiral arms. It exhibits a mottled appearance, potentially indicating regions of differing star formation activity or dust obscuration. The overall color of the disk is bluer compared to the bulge, indicative of younger, hotter stars. The galaxy does not appear significantly disturbed or interacting with another system. The overall morphology is indicative of a late-type spiral galaxy.
