The galaxy presents as a largely elliptical or spheroidal structure. It is relatively smooth in appearance, lacking any prominent spiral arms or strong indications of a disk component. There are no obvious signs of tidal disturbances or ongoing mergers with other galaxies. The color profile suggests a dominant population of older stars, exhibiting a yellowish-orange hue, indicative of lower star formation activity. The galaxy appears to be a mature system with an evolved stellar population.
