The galaxy presents as an elliptical or lenticular-like morphology, exhibiting a high degree of smoothness in its light distribution. The central region is characterized by a bright, concentrated bulge, suggesting a significant population of older stars. Moving outwards from the core, a more diffuse disk is present, though not displaying well-defined spiral arms. There is some indication of blue light in the outer regions of the disk, potentially indicating regions of ongoing, though likely moderate, star formation. The overall color of the galaxy shifts from yellow-white in the core to a slightly bluer hue in the outer regions. The isophotes appear mostly regular and elliptical in shape, without strong evidence of significant tidal disturbances or ongoing major mergers, though there may be some minor asymmetry.
