This galaxy presents an elongated, flattened disk structure, viewed nearly edge-on from our vantage point. A prominent central bulge is visible, exhibiting a smooth, concentrated light profile with a yellowish hue. The disk itself appears somewhat thicker towards the bulge, gradually thinning out as it extends outwards. Evidence of dust lanes or patchy extinction is discernible along the disk, suggesting the presence of obscuring material. The galaxy does not exhibit any obvious signs of strong tidal interactions or major mergers, although there appears to be some minor disturbances in the disk. Overall, the galaxy's morphology suggests a relatively evolved system, likely with a significant population of older stars contributing to its observed color.
