The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellow-white hue, suggesting a population of older stars. The light gradually fades outwards with a subtle color shift towards redder tones in the outer regions. No distinct spiral arm structures or bar features are discernible. There are no obvious signs of tidal disturbances, ongoing mergers, or significant star-forming regions, resulting in an overall elliptical appearance. The galaxy's light distribution appears relatively symmetrical. The object is compact with a high degree of roundness.
