The galaxy presents as an elliptical or lenticular morphology, appearing largely smooth and featureless. The central region exhibits a strong concentration of light, suggesting a prominent galactic bulge. The light from the bulge appears yellow-ish, potentially indicating an older stellar population dominating this region. Moving outward from the center, the light appears to fade with increasing radius and redden slightly, hinting at changes in stellar populations with increasing distance from the center. There are no distinct spiral arms or other disk-like features visible. Overall, the galaxy appears to be relatively undisturbed, showing no signs of ongoing major mergers or tidal interactions. The size of the galaxy suggests that it is a medium-sized system. Star formation appears to be quite low within the galaxy. The generally elliptical shape suggests random stellar orbits, and the light profile is consistent with a spheroidal galaxy.
