The galaxy presents a generally smooth and elliptical morphology. Its central region exhibits a high degree of luminosity, with intensity decreasing gradually towards the outer edges. The galaxy appears to be primarily composed of older stellar populations, indicated by its yellow-reddish hue. There is no indication of distinct spiral arms, a prominent disk, or significant dust lanes. The shape is predominantly in between round and elliptical. There is no visual evidence of an ongoing major merger event, but a minor disturbance or interaction cannot be ruled out based on this image alone. Overall, the galaxy appears to be a relatively evolved system.
