The galaxy presents an elliptical morphology, with a smooth light distribution emanating from its core. There is no substantial evidence of spiral arms or other disk-like structures. The central region exhibits a bright concentration of light, indicating the presence of a substantial galactic nucleus. Faint features suggest possible tidal disturbance in the structure, but this requires further investigation. The color gradient appears consistent across the galaxy, without notable blue components or other regions of star formation. The overall appearance suggests the galaxy is likely a passively evolving system.