The observed galaxy appears to be a spiral galaxy viewed nearly edge-on. A prominent dust lane bisects the galaxy along its major axis, obscuring the light from the galactic bulge. The bulge appears relatively bright and centrally concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. The disk of the galaxy is faintly visible extending outwards from the bulge, with indications of spiral arm structure. The spiral arms are diffuse and not sharply defined, exhibiting a mottled appearance with blueish and reddish colors, likely indicating ongoing star formation regions. Overall, the galaxy appears to be relatively undisturbed, showing no significant signs of a major merger, although some minor disturbances cannot be ruled out.
