The galaxy presents as a relatively bright, somewhat diffuse, elliptical or lenticular system. The central bulge is prominent and exhibits a yellowish hue, suggesting a population of older stars. The outer regions display a fainter, bluer tint indicating the presence of younger stars. The overall shape is moderately elongated. There appears to be a faint disk-like structure, but no clear spiral arms are discernible. There's a subtle asymmetry in the outer regions, possibly indicating past or ongoing minor gravitational interactions. Overall, it seems to be a massive galaxy with moderate star formation activity.
