The galaxy presents as an elliptical system, exhibiting a smooth, featureless morphology. Its light profile suggests a concentrated bulge with a significant spheroidal component. The color gradients indicate a generally old stellar population, with a yellowish hue dominating the central regions. There is some presence of blue color in a very small portion of the halo, indicating a very small amount of star formation. The overall form is slightly elongated, deviating moderately from perfect circularity. No prominent signs of tidal disturbances or ongoing major mergers are observed, although a slight asymmetry hints at a possible minor interaction in its past. The galaxy's estimated size suggests it is relatively massive, likely of the order of billions of solar masses.
