The galaxy presents as a largely homogenous elliptical structure, exhibiting a high degree of central concentration. The luminosity profile appears smooth, with no obvious spiral arm structures or prominent dust lanes visible. The overall color is yellowish-orange, suggesting an older stellar population dominated by redder stars. The morphology leans toward a spheroidal shape, although there is a slight deviation. Indications of minor disturbances exist, but the galaxy appears largely unperturbed. There is a slight color gradient visible from core to edge; it seems to be bluer towards the edge.
