The galaxy appears as a centrally concentrated object with a relatively smooth morphology. It exhibits a dominant, nearly spherical bulge. The galaxy's overall color leans towards the redder end of the spectrum, particularly in its central region, suggesting an older stellar population. Faint hints of a disk-like structure are potentially present but indistinct, and the galaxy is generally undisturbed, showing no signs of significant recent mergers or major tidal interactions. There may be very subtle diffuse features extending outward from the main body. Overall, the galaxy presents itself as a mature, early-type system with minimal ongoing star formation.
