The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated central bulge. Its color is a warm yellow-white, suggesting an older stellar population with minimal ongoing star formation. There is a slight elongation to the structure, though it is generally quite round. No spiral arms or obvious disk features are discernible. There are no strong indications of recent or ongoing major merger activity or tidal disturbances. The galaxy seems to be relatively isolated, exhibiting a well-defined, regular shape.
