The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge with a gradually decreasing light profile towards the outer regions. No distinct spiral arms or bar structures are visible. The overall color appears to be somewhat red, suggesting an older stellar population with fewer young, blue stars. There may be a minor tidal disturbance or faint plume suggesting a past or ongoing interaction with another galaxy, but this is relatively subtle. The morphology indicates this is likely a massive galaxy, but may have some level of star formation activity occurring. The galaxy appears to have a very high degree of rotational symmetry.
