This galaxy presents a flattened, disk-like morphology, viewed at a considerable angle, indicating a likely spiral or lenticular classification. The central region exhibits a bright, concentrated bulge, appearing smooth and slightly yellowish, suggesting a population of older stars. The galactic disk displays a blueish hue, more prominent in some regions than others. This suggests ongoing star formation, possibly concentrated within spiral arm structures that are not clearly resolved in this image, but are implied by the irregular distribution of the blue color. There is a small visual disturbance on the right side of the image; this could indicate a very faint tidal feature or a minor interaction with a smaller object. Overall, the galaxy appears relatively isolated and undisturbed, with a moderate rate of star formation occurring within its disk.
