The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that transitions into a fainter, more diffuse halo. There is some evidence of a subtle disk-like structure, but it is not highly pronounced. Color gradients suggest that the central regions are dominated by older stellar populations, with a yellowish hue, while the outer regions display slightly bluer tones. Overall, the galaxy seems to be undergoing little ongoing star formation. There may be some minor gravitational disturbances or interactions occurring, but it seems to be a relatively isolated system.
