The galaxy presents as a roughly elliptical disk, viewed edge-on or at a high inclination. A distinct central bulge region is present, exhibiting a bright, concentrated luminosity. The disk appears flattened and extended, with potential dust lanes visible as darker regions obscuring the starlight on either side of the central bulge. There are suggestions of disrupted morphology in the disk, potentially indicating tidal interactions or minor disturbances. The central region shows a distinct color variation, with a bright and possibly active galactic nucleus (AGN). The overall color suggests a mix of stellar populations, possibly with some ongoing star formation, although the limited resolution makes it difficult to assess the exact details of the disk's structure and composition.
