The galaxy presents as a disk-shaped system, seen at an oblique angle, and appears significantly elongated. The central bulge exhibits a higher surface brightness than the surrounding disk. The disk itself displays a relatively smooth texture with no distinct spiral arm structures discernible in the image. The overall light distribution suggests a relatively high degree of concentration towards the center. A slight asymmetry in the outer regions of the disk may indicate minor gravitational interactions or disturbances. The color profile appears to be relatively uniform throughout the galaxy, with a slightly redder hue.
