The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish in color, potentially indicating an older stellar population. There is a slight color gradient from the center outwards, with the outer regions appearing somewhat redder, which could indicate a less active star formation rate in these areas. No distinct spiral arms or bar structures are discernible. The overall shape is predominantly round, with no significant asymmetries or tidal disturbances visible, suggesting a lack of recent major merger events. The galaxy appears to be a fairly isolated system.
