The galaxy presents as a relatively smooth, elliptical morphology. There is a slight elongation in its shape, appearing more in-between round and cigar-shaped. No distinct spiral arm structures are discernible; the light distribution is centrally concentrated. There is little evidence of major disturbances or ongoing merger activity. The galaxy exhibits a subtle red color, potentially indicating an older stellar population and reduced star formation activity. There is also a possible, very faint tidal tail.