The galaxy presents as a centrally concentrated object with a smooth morphology. There is some indication of a subtle, disk-like structure, however, the overall appearance is dominated by a spheroidal component. The light distribution exhibits a gradual decline from the center outwards, showing no strong spiral arm features or bar structures. The color profile indicates a redder population, suggesting an older stellar population with minimal active star formation. While there are no signs of major interactions or ongoing mergers, a slight asymmetry in the outer regions might suggest a minor disturbance or tidal interaction in the past.
