This galaxy presents as a spiral type, oriented approximately face-on with a notable central bulge. The bulge exhibits a yellowish-orange hue, suggesting a population of older stars. Two tightly wound spiral arms emanate from the bulge region, displaying a bluer color indicative of ongoing star formation. The spiral arms are not perfectly symmetrical, showing some irregularities and patchy distribution of star forming regions. The bar appears to be quite prominent. Overall, the galaxy has a disk structure and has not recently undergone any major mergers.
