The galaxy presents a morphology consistent with a spiral type. The disk is viewed at an angle that is closer to face on rather than edge on. The central bulge is moderately sized and presents a yellowish-white color, indicating an older stellar population. Faint spiral arms extend outwards from the central bulge. The arms are populated with regions of blue light, suggestive of ongoing star formation. There is no obvious strong bar feature, but the inner regions of the disk may present a weak bar like structure. The disk itself is relatively smooth in appearance, though there is some mottled texture indicating substructure. There is no obvious strong tidal features or evidence of a major merger event, but there is an apparent irregular distribution of light within the disk that may suggest a minor disturbance event.
