The galaxy appears to be a lenticular or early-type spiral galaxy, viewed at an oblique angle relative to its disk plane. It exhibits a somewhat flattened, elliptical morphology, with a central bulge region that appears relatively smooth and bright. The disk component is subtly visible, with a slight extension on either side of the bulge. The overall color is moderately blue-white, suggesting a population of young to intermediate-age stars is present within it. There does not appear to be a large amount of dust in the galaxy, as there are no prominent dust lanes visible in the image. There also appears to be some distortion or asymmetry in the galaxy's shape. This could indicate a past or ongoing minor merger event. There is no visible active galactic nucleus. Given the galaxy's apparent size and lack of resolved features, it is likely a considerable distance away. Overall, the galaxy seems to be an intermediate-mass system with a low star formation rate.
