The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth, amorphous structure with a bright, concentrated central bulge. A faint disk-like structure is potentially visible, but it's heavily obscured by the overall smoothness and lack of defined spiral arms. The galaxy shows a warm color, primarily concentrated in the bulge, indicating an older stellar population. Minor disturbances may be present, possibly indicating a recent interaction or merger event. The system appears to be experiencing a low rate of star formation, consistent with the dominant presence of older stars in the bulge.
