The galaxy appears to be a spiral galaxy observed at a redshift of approximately 0.15, suggesting a considerable distance. It presents a disk-like structure with prominent spiral arms. The arms are relatively tightly wound. There is a distinct central bulge that is moderate in size, with a bright yellow-orange hue, possibly indicating a population of older stars. The spiral arms exhibit a bluer color, suggestive of ongoing star formation. Two main arms are visible, extending from the bulge. There is no obvious bar structure present. No signs of major mergers or significant disturbances are readily apparent. The overall light from the galaxy is consistent with a high mass and intermediate star formation rate.
