The galaxy presents as a spiral type, with tightly wound spiral arms emanating from a moderately sized central bulge. The spiral structure is dominant, occupying a substantial portion of the galactic disk. The arms exhibit a patchy, somewhat flocculent morphology, suggesting active regions of star formation. The bulge appears relatively smooth and concentrated, with a color profile indicative of an older stellar population. There are some minor disturbances that may be attributed to interactions with smaller objects. Overall, the galaxy displays a fairly well-defined disk structure with notable spiral arm features.
