The galaxy presents as a moderately bright, elliptical-like object, exhibiting a smooth, diffuse morphology. Its color profile indicates a concentration of older stellar populations toward the core, suggested by the yellowish-white hue in the central region. Fainter blue hues extend away from the center. The galaxy displays no obvious spiral arm structure. There is a slight elongation in its shape, deviating from a perfect circular form. The lack of prominent dust lanes or patchy star-forming regions further supports its classification as an elliptical or lenticular galaxy. The galaxy's overall light distribution appears to be centrally concentrated, indicative of a bulge-dominated system.
