This galaxy presents as an edge-on spiral, exhibiting a flattened disk structure. A pronounced central bulge dominates the galaxy's luminosity, displaying a smooth, rounded morphology. The disk appears relatively uniform in color, with some subtle variations in intensity along its length. The galaxy's overall color index suggests a population of older stars and potentially a reduced rate of on-going star formation within the disk. No prominent dust lanes or distinct spiral arm structures are discernible at this resolution, indicating a likely evolved state or a lack of significant interstellar medium obscuration. There's no indication of ongoing major merger activity, though subtle disturbances may exist.
