This galaxy presents as a face-on spiral system. The central bulge exhibits a yellow-orange hue, indicative of an older stellar population. Prominent spiral arms extend from the central region. These arms display a patchy, blue-ish color, suggesting ongoing star formation. There appears to be a bar structure through the central region, which could be contributing to the apparent spiral arm morphology. The dust lanes, though not clearly delineated, hint at active regions within the arms. The spiral arms are well-defined and extend fairly far out. The overall morphology suggests a galaxy that is actively forming stars, with a relatively well-established spiral structure. It is unlikely to be undergoing any major mergers but may have minor disturbances.
