The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a higher surface brightness, appearing nearly spheroidal and more intensely luminous, possibly indicating a significant concentration of older stellar populations. Progressing outwards, the galaxy's light gradually fades, though a subtle color gradient is observable, transitioning from a warmer, yellowish hue in the center to a cooler, slightly bluer tint in the outer regions. The overall structure suggests minimal disturbance, lacking clear tidal features or signs of active merging events. The galaxy appears somewhat elongated but is generally round.
