The galaxy presents as a relatively compact, elliptical-like system with a smooth, centrally concentrated light distribution. A single concentration of light dominates. There is a gradual fading of light intensity from the center outwards, indicating a lack of distinct structural features such as spiral arms or a prominent bar. The color appears somewhat uniform, with a yellowish-white hue, suggesting a population of older stars. There is little evidence of ongoing star formation or significant dust lanes that are often associated with spiral galaxies. It appears that the galaxy is a relaxed system with minimal signs of recent merging activity or tidal disturbances. 
