The galaxy presents as a disk galaxy, observed nearly edge-on. The central bulge appears prominent and spheroidal, exhibiting a yellowish hue, possibly indicative of an older stellar population. A flattened disk extends outwards from the bulge, appearing relatively smooth with limited visible dust lanes or spiral arm structures. The disk displays a bluer tint compared to the bulge. The overall morphology suggests an evolved system, potentially undergoing a period of reduced star formation within the disk. No signs of major mergers or significant tidal disturbances are apparent in this image.