This galaxy presents as a flattened, disk-like structure seen nearly edge-on. It exhibits a bright, concentrated central bulge, suggesting a significant population of older stars or an active galactic nucleus. The disk component appears relatively smooth, with a noticeable lack of prominent spiral arms or distinct dust lanes. 

The color profile indicates a higher concentration of blue light within the central region, potentially signaling ongoing star formation. Fainter, diffuse emission extends outwards from the main body of the galaxy, forming a faint halo. There appears to be a slight asymmetry or disturbance in the outer disk region on the left side, suggestive of a minor gravitational interaction. The overall morphology suggests a possible lenticular or early-type spiral galaxy.
