The galaxy presents as a lenticular or early spiral type, exhibiting a prominent central bulge that appears relatively smooth and concentrated. The disk component is discernible, though less defined, showing a hint of spiral structure. The galaxy is elongated, appearing somewhat cigar-shaped rather than perfectly round, indicative of a possible edge-on or highly inclined orientation relative to our line of sight. There is evidence of a minor disturbance in the galaxy's morphology; a slight asymmetry and faint tidal features suggest the possibility of a past interaction or merger. A diffuse, low-level star formation may be present as suggested by slight colour variations along the disk. The galaxy’s overall color is consistent with an older stellar population, dominated by evolved stars, though some younger stars may also be present.
