The galaxy appears as a luminous, relatively smooth object. There is no apparent spiral structure or distinct disk. The light is centrally concentrated with a gradual falloff in intensity towards the outer regions, suggesting a spheroidal morphology. A slight elongation is observed, but the galaxy is largely symmetrical. It exhibits no obvious signs of recent major mergers or strong tidal disturbances. There is a faint hint of blue color, but it is predominantly composed of older stellar populations, and it presents a moderate level of star formation. The galaxy likely possesses a stellar mass of approximately 10^9.7 solar masses.
