The galaxy presents as a flattened, disk-like structure with a noticeable central bulge. The central bulge appears nearly spherical with a high surface brightness that fades outwards to the edge of the bulge. The disk component exhibits a subtle color gradient, transitioning from a bluer hue in the inner regions to a redder tint towards the outer edges. There are suggestions of spiral arms or similar features within the disk, but they are poorly defined. The galaxy's overall appearance suggests a relatively smooth structure with no major disturbances or obvious signs of interaction. There may be a low level of on-going star formation.
