This galaxy appears to be a relatively smooth, elliptical system. The light profile exhibits a central bulge that is bright and concentrated, with a color gradient trending toward yellow-orange in the innermost regions. This suggests an older stellar population in the core. Surrounding the central bulge is an extended, fainter halo. The halo shows a bluer hue, indicating the presence of younger stars. No distinct spiral arms or obvious dust lanes are visible. The overall morphology suggests that this galaxy is likely an early-type system undergoing a relatively low rate of star formation. There is no major disruption to the shape, indicating it is not undergoing a major merger. There is a slight asymmetry.