The galaxy presents a largely smooth morphology with a concentrated central bulge. There is faint evidence of a disk. The light is dominated by redder wavelengths with a concentrated, bright core. The surrounding halo of light is more diffuse, lacking any well-defined spiral arm structures. The shape of the galaxy is approximately round, though there is some slight elongation. No signs of any major mergers or tidal disturbances are immediately visible, but there may be some minor interaction. Overall, the galaxy is a mature system with relatively low star formation activity, with redder stellar populations.
