The observed galaxy exhibits a pronounced spiral structure. The spiral arms appear somewhat tightly wound around a moderate-sized central bulge.  The galaxy is not viewed edge-on, allowing for clear observation of its spiral morphology.  While distinct spiral arms are visible, there is an element of fuzziness, potentially indicating the presence of significant dust obscuration, or possibly a lower resolution.  The overall color suggests a population of older stars dominating the bulge. There may be signs of some minor interaction, with what could be minor disturbances.
