This galaxy presents as an edge-on spiral galaxy, exhibiting a prominent disk structure. A significant dust lane bisects the galaxy, obscuring a substantial portion of the galactic plane and contributing to the apparent reddening of the light. The central bulge appears to be rounded and diffuse, lacking sharp definition, with a concentration of light suggestive of an older stellar population. There is no evidence of a recent or ongoing major merger event. The disk appears relatively undisturbed, although subtle irregularities may indicate minor disturbances. The overall color suggests a mix of stellar populations.
