The galaxy exhibits a disk-like morphology, observed at a significant inclination, tending towards edge-on. It displays a central bulge region that appears relatively prominent and concentrated, exhibiting a yellowish hue, potentially indicating an older stellar population. The surrounding disk component shows a bluer color, suggesting ongoing star formation. The disk appears moderately disturbed with some hints of internal structures. There is a lack of any signs of a major merger or significant tidal disruptions.
