The galaxy presents as a spiral type, with a prominent central bulge. The spiral arms are relatively tightly wound and moderately defined, emanating from the central region. The disk is viewed at a slight angle, not perfectly face-on. The bulge appears to be of moderate size in relation to the overall galactic disk. There is no evidence of major mergers or significant tidal disturbances. The structure is overall dominated by the spiral pattern, rather than a smooth, elliptical appearance. The galaxy has blue tinges to it indicating star formation. 