The galaxy exhibits a primarily smooth morphology with a slight ellipticity, appearing as an intermediate shape between round and elongated. There is a central bulge with a high surface brightness, surrounded by a fainter, more diffuse halo. The color gradient suggests an older stellar population throughout, with a hint of slightly bluer hues further from the center, potentially indicating recent, but limited, star formation in the outer regions. There is no strong evidence of spiral arm structures or significant dust lanes. A very minor disturbance may be occurring, or recently occurred, due to the asymmetries in the halo, but nothing significant is noticed.
