The galaxy appears to be an elliptical galaxy, exhibiting a smooth, generally featureless morphology. The central region displays a high concentration of light, with a gradual decrease in luminosity outwards. The overall shape is close to circular but not perfect, with a slight elongation observed. There may be some minor disturbances based on the ragged shape of the outer halo, but overall, the structure is relatively undisturbed. There is no clear evidence of spiral arms, dust lanes, or a prominent disk component. The galaxy is composed of older stars with a low star formation rate. The mass of this galaxy is significant.
