The galaxy presents a predominantly smooth morphology, with a relatively high degree of roundness. A slight asymmetry is apparent, with a faint, extended feature visible on one side, suggestive of a potential tidal interaction or disturbance. The galaxy exhibits a distinct color gradient, with a centrally concentrated yellowish-white core, transitioning to bluer hues in the outer regions, indicative of varying stellar populations and star formation activity. Overall, the galaxy appears to be a relatively massive system, likely an early-type spiral or lenticular galaxy undergoing some form of interaction or internal process influencing its morphology and stellar distribution.
