The galaxy presents as a concentrated spheroid, exhibiting a relatively smooth morphology with a dominant central bulge. The color gradient transitions from a yellowish-white core to a diffuse, slightly bluer outer halo. While largely smooth in appearance, a subtle, faint disk-like structure may be present, though it lacks distinct spiral arm features. There is no strong evidence of ongoing or recent major merger activity; however, slight asymmetry and a potential tidal tail hint at minor disturbance or a past interaction. The galaxy exhibits a notable red-shift, suggesting substantial distance and significant luminosity. The overall light profile suggests an evolved stellar population, consistent with a low specific star formation rate. The galaxy is moderately massive.
