The galaxy presents as an elliptical morphology, with a smooth, concentrated central bulge that is slightly elongated in shape. The light distribution appears fairly uniform, with a gradual fading from the core outwards into the surrounding halo, showing no distinct arms or spiral structure. The overall color is relatively red, suggesting an older stellar population, yet there appears to be a subtle bluer hue around the central bulge. This suggests the presence of a small population of younger, hotter stars in the central region, possibly indicative of recent star formation. There are no signs of any significant tidal disturbances or interactions with neighboring galaxies. Overall, the galaxy seems to be a well-formed, relatively undisturbed system.
