The galaxy presents as a disk-dominated system, observed nearly edge-on. A prominent dust lane bisects the galaxy, obscuring a significant portion of the central bulge region. The bulge appears relatively small. The overall color suggests a mix of stellar populations, with bluer hues indicative of younger stars in the disk and redder tones potentially associated with an older stellar population in the bulge and/or dust extinction. There is some asymmetry visible in the dust lane which might indicate past disturbance or interaction. The disk appears relatively smooth.
