The galaxy appears to be a spiral type, viewed at an angle that is nearly face-on. A prominent central bulge dominates the morphology, with a moderate size relative to the overall disk. The spiral arms are readily apparent, displaying a grand design structure, characterized by relatively tight windings. Two major arms extend from the central region, exhibiting a clear symmetry. There are some indications of ongoing star formation within the arms, as suggested by subtle variations in color and texture. There does not appear to be a strong bar feature bisecting the central bulge. The galaxy is overall symmetrical and organized, showing no clear signs of major mergers or significant tidal disturbances.
