The galaxy presents as a flattened, disk-like structure with a significant degree of inclination relative to our line of sight. The central bulge region appears relatively smooth and concentrated, exhibiting a yellowish-orange hue indicative of an older stellar population. Moving outward from the center, the disk shows a subtle fading of light, and is also slightly redder, with some dust obscuration, but lacks distinct spiral arm structures. The apparent high inclination limits a detailed analysis of features within the galactic plane. The overall morphology suggests a possible late-type spiral galaxy, though the absence of prominent spiral arms could indicate a more lenticular or transitional classification.
