The galaxy presents as a flattened, elongated structure, suggestive of a disk galaxy viewed at a high inclination. The central bulge appears relatively prominent and exhibits a yellowish-white hue, potentially indicative of an older stellar population. The disk, extending outwards from the bulge, shows a subtle gradient in color, transitioning from the yellower central region to fainter, bluer edges. There is a faint, diffuse glow surrounding the galaxy, possibly a halo of older stars or scattered light. Subtle disturbances in the disk's morphology are visible, possibly indicating minor gravitational interactions or internal processes affecting its structure. The overall appearance suggests a galaxy with a significant mass, but low rate of star formation.
