This galaxy exhibits a well-defined spiral structure. Two prominent spiral arms emanate from a central bulge. The arms appear tightly wound around the bulge. The bulge is small compared to the overall size of the galaxy and it seems to have a higher concentration of older stars, indicated by the yellowish or white coloration at the core. The spiral arms display bluer hues, indicative of ongoing star formation activity, as expected. Overall, the galaxy appears to be relatively undisturbed, showing no obvious signs of major mergers or tidal interactions.
