The galaxy appears as a centrally concentrated object with a generally smooth morphology. The central region exhibits a bright, somewhat compact core. Surrounding this core is a more diffuse, extended halo of light. There are subtle color gradients apparent, with the core exhibiting a slightly redder hue, potentially indicating an older stellar population. The outer regions of the galaxy show a hint of bluer tones, which could be indicative of more recent or ongoing star formation in those areas. The overall shape is largely spheroidal. There is little to no evidence of strong spiral arm structure or other pronounced morphological features associated with disk galaxies. There is minimal, if any, evidence of major tidal disturbances or ongoing mergers, though subtle asymmetry or faint extensions cannot be ruled out.
