The galaxy presents as a flattened, disk-shaped structure, viewed nearly edge-on. A prominent central bulge exhibits a smooth, concentrated luminosity profile, suggesting an older stellar population dominating the core. The bulge appears spheroidal in shape. The disk component, while not highly resolved, indicates the presence of a stellar population extending beyond the central bulge. The galaxy does not show strong signs of ongoing major mergers or tidal disturbances in this image. The disk is oriented at a steep angle with respect to our line of sight, potentially obscuring detailed features. The light from the disk appears to be generally smooth and uniform.
