The galaxy presents as a largely featureless elliptical or lenticular galaxy. It displays a high degree of central concentration, with a bright core that gradually fades into a diffuse halo. The overall shape is nearly circular, with a slight suggestion of elongation along its major axis. There is a subtle color gradient, shifting from a whiter core to a slightly redder periphery. There are no clearly defined spiral arms or dust lanes. There is no evidence of active star formation, and the galaxy appears to be dominated by an older stellar population. There is no distinct nucleus. Subtle irregularities in the outer halo suggest possible past interactions or minor disturbances. The galaxy appears relatively isolated, with no immediate companions visibly disrupting its morphology.
