The galaxy appears as a single, centrally concentrated object with a largely smooth morphology. There is little evidence of spiral arms or significant dust lanes. It exhibits a generally elliptical or spheroidal shape, appearing quite rounded. The color profile suggests a dominant population of older stars with the characteristic yellowish/reddish hue. There is no obvious sign of a recent major merger event or tidal distortions in the galaxy's structure. The light is rather evenly distributed, with the brightest emission concentrated in the central bulge of the galaxy. There may be some hint of an extended halo but it is poorly defined.
