The galaxy presents as a centrally concentrated, elliptical-like structure. Its light distribution appears relatively smooth, lacking prominent spiral arms or distinct features. The core is a bright, somewhat concentrated region, suggestive of an older stellar population. The color profile grades outward from a yellowish-white core to redder hues in the outer regions. There is a slight asymmetry in the galaxy's shape, but no indications of major disturbances or recent merger activity. The galaxy's overall appearance suggests a relatively quiescent system that is transitioning to more of a stable state.
