The galaxy presents as an elliptical structure with a smooth, concentrated central bulge. The light profile appears relatively uniform, lacking prominent spiral arms or distinct dust lanes. The core region exhibits a bright, yellowish hue, possibly indicating an older stellar population. The outer regions of the galaxy transition to a slightly bluer color, suggesting the presence of younger stars, but the color gradient is subtle. The overall shape is nearly circular, with no signs of significant tidal disturbances or ongoing major mergers. There are suggestions of minor irregularities or faint features in the disc region but they are so subtle as to not be definitive of any structure. The galaxy displays a moderate overall luminosity.
