The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity that appears to be slightly red-shifted, potentially indicating an older stellar population. There's a subtle colour gradient observed moving outward from the core, with a slight shift towards bluer wavelengths at the galaxy's edges. This could imply regions of more recent, albeit subdued, star formation in the outer areas, as the blue light of younger stars is more prominent than the red light of older stars.

The overall shape appears close to circular, and there is little visual evidence of significant tidal disturbances or ongoing major mergers. Any indications of spiral arms or distinct disk features are absent. There is a faint, diffuse halo surrounding the primary body of the galaxy, suggesting a more extensive and tenuous distribution of stars and potentially dark matter.
