The galaxy presents as a generally smooth, elliptical structure with a slightly elongated morphology. There is a central, brighter region which likely constitutes the galactic nucleus. Moving outwards, the light gradually diminishes into what seems to be a homogenous galactic halo. The colour profile indicates a light blueish-white hue, which fades into a redder tinge towards the outer edges. There are no obvious signs of spiral arms or significant dust lanes. There is a very slight hint of asymmetry, but this is not definitive, and could be due to limitations in image resolution or potentially minor disturbances. Overall, the galaxy appears to be relatively undisturbed, with a more quiescent star formation rate.
