The galaxy presents a generally elongated, disk-like morphology, observed at a significantly inclined angle. The central bulge is prominent, exhibiting a concentrated, smooth appearance with a yellowish hue, likely indicative of an older stellar population. Moving outward from the bulge, the disk shows a complex structure with subtle variations in brightness and color. One side of the disk appears slightly extended and possibly warped. There is a faint bluer section towards the edge that might indicate on-going star formation in this area. Some disturbances are present within the disk, and it's likely the galaxy is either undergoing, or has undergone, a minor merger event. The system exhibits moderate luminosity with a range of stellar ages evident from the color gradients across its structure.
