The galaxy exhibits a slightly elongated morphology, appearing neither perfectly spherical nor highly flattened. There is a moderate concentration of light towards the center, indicating a bulge component, but the light distribution is not entirely smooth. Faint features or irregularities are present, possibly indicative of internal structure or gravitational interaction. The galaxy's color suggests a mix of stellar populations, as both bluer and redder regions can be discerned. The overall appearance leans towards a somewhat disturbed or dynamically active system. The possibility of a minor merger or tidal disturbance cannot be ruled out based on the observed morphology.
