This galaxy appears to be a spiral galaxy viewed at an oblique angle. The central bulge is prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter spiral arms extend from the bulge, displaying a bluer tint, possibly indicative of younger stars and ongoing star formation. The disk appears relatively thin and there is some indication of dust lanes within the disk. There may be evidence of minor disturbances in the galaxy's structure, but it is primarily a single, distinct object with no significant signs of merging activity.
