The galaxy presents as an elongated, spindle-like structure with a significant central bulge. The core exhibits a yellowish hue, possibly indicative of an older stellar population. Moving outward from the central region, the color transitions to a bluer tone, hinting at ongoing star formation within the galactic disk. The disk structure shows some clumpy regions and a subtle degree of irregularity, suggesting a degree of internal disturbance or interaction. No obvious spiral arm structures are discernible from the image. The galaxy possesses a relatively smooth overall appearance, with no clear signs of a recent major merger.
