This galaxy presents as a spiral, viewed at a slight angle that is not quite edge-on. The disk is prominent and shows distinct, well-defined spiral arms. A strong, bright central bulge is apparent, with a moderate size relative to the overall disk. The winding of the spiral arms appears to be of medium tightness. Two main spiral arms can be distinguished. There is no obvious evidence of a strong bar structure, although a faint, elongated central feature might suggest a weak bar. Overall, there is no clear indication of any major ongoing mergers, or large disturbances, although a minor perturbation cannot be ruled out.
