The galaxy presents as a spiral type, with well-defined, tightly wound spiral arms. The arms exhibit a granular texture, suggesting regions of active star formation within them. The central bulge appears prominent and moderately sized, exhibiting a smooth, concentrated light profile, indicative of an older stellar population. There is no apparent strong bar structure bisecting the bulge, but a subtle asymmetry or slight elongation within the central region might suggest a weak bar. The overall disk inclination is moderate, allowing for a clear view of the spiral arm structure. There is no immediately obvious indication of a major ongoing merger event.
