The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse appearance, likely an elliptical morphology. It exhibits a dominant yellowish-white hue in its core, suggesting an older stellar population and relatively low star formation activity. The isophotes appear generally round, although there is a subtle elongation along one axis, possibly indicating a slight departure from perfect sphericity. There is no obvious evidence of spiral arms, dust lanes, or recent merger activity. The outer regions of the galaxy fade smoothly into the background, with no sharp truncation or clear boundary observed.
