This galaxy exhibits a predominantly smooth morphology, appearing as an elliptical structure. The central region displays a concentrated luminosity, suggesting a dense stellar population or a possible active galactic nucleus. The outer regions fade gradually, indicating a decreasing stellar density with increasing radial distance from the core. There are hints of a subtle disk-like structure, although the smoothness dominates. Minimal signs of strong tidal interactions or major disturbances are apparent. The color profile reveals an overall redder hue, suggestive of an older stellar population with reduced active star formation. There may be minor evidence of disturbed morphology with possibly slight distortions in its shape. 
