The galaxy presents a disk-like structure with a noticeable central bulge. The bulge appears relatively prominent and moderately bright, with a yellowish hue, suggesting an older stellar population. The disk component is viewed at a moderate inclination, allowing some structural details to be observed. Faint spiral arms are tentatively visible extending outwards from the central bulge. These arms appear patchy and somewhat poorly defined, hinting at ongoing, but perhaps not vigorous, star formation. The outer regions of the disk fade gradually, indicative of a decreasing stellar density. Overall, the galaxy exhibits a well-defined structure with a combination of bulge and disk characteristics. No obvious signs of recent major merger activity or significant tidal disturbances are apparent, though minor disturbances are not ruled out.
