The galaxy presents an elliptical morphology, with a smooth, concentrated light profile. The central region exhibits a bright, yellowish-white core, suggesting an older stellar population dominating that area. Moving outwards, the galaxy's color gradually shifts to a more muted yellow, indicating potentially less star formation in the outer regions. The galaxy appears relatively undisturbed, lacking any significant signs of tidal interactions or major mergers. There is a subtle suggestion of a flattened structure, possibly indicative of a disk component, but the overall appearance is predominantly spheroidal. There are no apparent dust lanes or spiral arms visible in this image. The light is generally smooth and even with no evidence of current star formation. It is likely this galaxy is undergoing very little star formation and is thus composed of older stars.
