The galaxy presents as a face-on spiral structure with a notable central bulge. The spiral arms are clearly defined, exhibiting a moderate winding pattern. The disk component appears to be the dominant feature with a yellow orange hue, punctuated by regions of lighter concentrations in the outer arms, potentially indicative of active star forming regions. The central bulge presents a smooth appearance and intense coloration, suggesting a well-established population of older stars. There is a noticeable lack of significant dust lanes or complex features within the spiral arms, which would otherwise indicate ongoing disturbances or interactions. Overall, the galaxy appears to be a relatively undisturbed system, with a dominant disk and a moderate bulge component.
