The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It presents with a moderate ellipticity, exhibiting an elongated, cigar-like shape. The light distribution is concentrated toward the center, displaying a bright, relatively uniform bulge. Fainter, diffuse emission extends outwards from the core region, with a subtle gradient in surface brightness. There's a slight suggestion of a disk-like structure, though this is not clearly defined. No distinct spiral arms or prominent dust lanes are visible. There may be a very minor tidal disturbance that is faintly visible, however it is not certain. The galaxy appears to be relatively isolated, with no clear signs of a major ongoing merger event. The overall color appears redder, suggesting an older stellar population and a lower rate of star formation.
