The galaxy presents as a relatively smooth, disk-like structure seen at an oblique angle. There is a slight elongation, suggesting a flattened morphology. Color gradients are apparent, with a yellowish-orange hue more concentrated towards the central region, indicating a population of older stars. The outer regions appear slightly bluer, possibly indicating areas of more recent, albeit subdued, star formation. No distinct spiral arm structures are discernible in the image. Overall, the galaxy appears relatively undisturbed, with no immediately obvious signs of ongoing major mergers or tidal interactions. The galaxy's apparent size is relatively small, suggesting a moderate physical dimension.
