The galaxy presents as a somewhat smooth, lenticular or early-type spiral galaxy with a slight inclination to our line of sight. Its color profile is mostly reddish-gold, potentially indicating an older stellar population and/or significant dust obscuration. There is a hint of bluer regions toward the edges of the galaxy, implying the presence of younger stars. The structure appears mostly undisturbed, lacking significant tidal tails, mergers or other major disturbances, though very subtle disturbances or possible minor companions cannot be fully ruled out at this resolution. Its elongated shape suggests it is not perfectly spherical.
