The galaxy presents as a spiral galaxy, viewed at an angle. The galactic bulge is moderately sized and displays a yellowish hue, suggestive of an older stellar population. The spiral arms are not highly defined, but appear tightly wound around the central bulge. Faint blue regions may trace areas of ongoing star formation within the arms. No strong bar structure is apparent. The disk is relatively smooth, with no clear indication of significant morphological disturbance or a major merging event. Overall, it appears to be a relatively quiescent galaxy.
