The galaxy appears to be an elliptical or lenticular type. It exhibits a smooth, centrally concentrated light distribution with a slight elongation, suggesting a cigar-shaped morphology. The core region displays a reddish hue, potentially indicating an older stellar population. The outer regions show hints of a flattened disk-like structure, though this is not as prominent as in spiral galaxies. There is no visible evidence of recent or ongoing major mergers or significant tidal disturbances. The overall color suggests a lack of substantial star formation, which aligns with the galaxy's generally smooth and evolved appearance.
