The galaxy appears to be a relatively smooth, elliptical or lenticular type, exhibiting a high degree of central concentration. The dominant feature is a bright, diffuse bulge, possibly indicating an older stellar population. There is very little evidence of spiral arms or significant disk structure. The galaxy appears largely featureless, lacking prominent dust lanes or star-forming regions. The overall round shape suggests that it is viewed close to face-on. There is no obvious signs of any major disturbances, interactions or mergers.
