The galaxy presents an elongated, disk-like morphology, viewed nearly edge-on. A prominent central bulge dominates the galaxy's core, exhibiting a smooth, concentrated distribution of light. The disk appears relatively thin. Dust lanes are not readily apparent but may exist within the plane of the disk. The galaxy appears redder towards the center of the bulge, and blue along the disk. There is no evidence of strong spiral arm structures or active star formation regions. The overall color suggests an older stellar population, consistent with a relatively quiescent star formation history. The absence of significant tidal features or distortions suggests a dynamically relaxed system.
