This galaxy exhibits a clear spiral structure. The spiral arms appear tightly wound, originating from a central bulge that seems moderately sized in relation to the overall disk. The bulge exhibits a yellowish hue, indicative of an older stellar population. The spiral arms show a bluer color, suggesting ongoing star formation. The galaxy appears to be relatively undisturbed, lacking strong indications of recent major mergers or tidal interactions. The disk is viewed at a shallow angle, not quite face-on. There is no sign of a strong central bar. Star formation appears to be active but not extreme.
