This galaxy presents as a spiral galaxy with a well-defined disk structure. Distinct spiral arms are discernible, exhibiting a moderate winding pattern. The central bulge appears prominent but not dominant, exhibiting a yellow/white hue, indicative of an older stellar population. The disk displays a bluer colour, suggestive of ongoing star formation regions and a younger stellar population. There is no evidence of a strong bar structure. No major signs of tidal disturbances or merging events are apparent.
