The galaxy presents as a centrally concentrated elliptical type with a smooth, relatively featureless light distribution. The core exhibits a bright, yellowish hue, suggesting an older stellar population. The outer regions appear more diffuse and slightly redder in color. The galaxy appears nearly spherical, with only a slight elongation. There is some evidence of minor tidal disturbances or faint features extending outwards from the main body of the galaxy which could be a result of a minor merger. The overall morphology points towards a quiescent system, with limited ongoing star formation.
