The galaxy exhibits a disk morphology, presenting a notable inclination relative to our line of sight. Within the disk, spiral arm structures are visible, albeit somewhat diffuse and lacking sharp definition. The central bulge appears moderately sized, contributing significantly to the overall light profile. The bluer hues distributed throughout the galaxy suggest ongoing star formation activity. The galaxy shows no obvious signs of major interaction or merging events, however the lower region of the disk has a blobular appearence possibly indicating a minor disturbance or merger event. Overall, the galaxy can be categorized as a spiral galaxy with an actively star-forming disk and a moderately sized central bulge.
