The galaxy presents as a spiral type, with a well-defined disk structure. Prominent spiral arms are visible, exhibiting a relatively clear winding pattern. The central bulge appears moderately sized, characterized by a yellowish hue, indicating an older stellar population. The disk displays a bluer tint, suggesting ongoing star formation. A strong bar structure bisects the central bulge. Some disturbances or asymmetries are observed in the outer regions of the disk, potentially indicating minor gravitational interactions with other galaxies, or potentially from internal processes. The spiral arms are slightly flocculent. The galaxy does not appear to be edge-on.
