The galaxy presents as an edge-on spiral with a prominent central bulge. The bulge appears relatively smooth and exhibits a yellowish hue, suggesting an older stellar population. A dust lane is discernible bisecting the galaxy, appearing as a dark band along the major axis. The disk shows bluer colors, indicative of ongoing star formation, and a slight degree of patchiness, implying some spiral arm structure. There appears to be little evidence of significant tidal disruption or major mergers, though a faint asymmetry on one side could indicate a minor interaction or disturbance. The galaxy is moderately luminous.
