The galaxy presents as a spiral type with a prominent disk structure viewed at an oblique angle. The central bulge appears moderately sized, with a yellow-ish hue suggesting an older stellar population. Two distinct spiral arms are observed extending from the central region, exhibiting a moderately wound structure. Patches of bluer light are noted along the spiral arms indicating regions of recent or ongoing star formation. A hint of a bar structure is suspected, potentially a weak or intermediate bar, based on a slight elongation in the central region. No obvious signs of major merger events are visible; the galaxy appears relatively undisturbed, though some minor irregularities or distortions within the disk cannot be ruled out. The overall color suggests a mixed stellar population, with both older, redder stars in the bulge and younger, bluer stars in the spiral arms.
