The observed galaxy exhibits a morphology consistent with a spiral galaxy viewed at a high inclination angle, approaching edge-on. A prominent central bulge, exhibiting a yellowish hue suggestive of an older stellar population, dominates the core region. The galactic disk appears flattened and elongated, with a blueish tint along what appears to be the upper edge. The dark regions may be due to the presence of dust lanes obscuring background starlight within the galactic disk. There is some faint asymmetry present in the disk, potentially indicating a past minor interaction or disturbance. No obvious signs of ongoing major merging activity are observed. 
