The galaxy presents as a singular, somewhat amorphous, and centrally concentrated light source. The overall morphology appears relatively smooth with an elliptical-like structure. The galaxy is not perfectly round, showing a slight elongation. There is no strong evidence of spiral arms or a well-defined disk component from this view.  There is no visually significant sign of major mergers or strong tidal disturbances. The galaxy appears to be relatively undisturbed. The color profile suggests a population of older stars, potentially lacking strong ongoing star formation.
