The galaxy presents as a disk-shaped structure, viewed nearly edge-on from our vantage point. A prominent central bulge is visible, exhibiting a smooth, luminous profile with a yellowish hue, suggesting a population of older stars. The disk itself appears relatively thin and elongated, displaying a subtle color gradient moving outward from the bulge. The outer regions of the disk appear fainter and bluer, indicating the potential presence of younger stars. There is no obvious evidence of strong spiral arm structure or active star-forming regions within the disk. No significant tidal features or signs of recent mergers are readily apparent.
