The galaxy presents as a fairly smooth and elliptical structure. There is a central bulge that appears bright and yellowish, indicating a population of older stars. The color becomes slightly redder towards the outer regions, perhaps suggesting a decline in recent star formation further from the center. The galaxy's overall form is quite regular, showing little evidence of ongoing mergers or major tidal disturbances. There may be a subtle disk-like component or faint spiral arms, but these features are not strongly pronounced. The galaxy appears relatively isolated in its immediate environment.
