The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution exhibits a notable radial gradient, with a bright, yellowish core that transitions smoothly into a fainter, bluish outer region. The overall morphology suggests a relatively evolved system, possibly an early-type spiral or lenticular galaxy. There is very little dust observed in this image. No strong spiral arm structures or prominent star-forming regions are discernible. The galaxy appears isolated, showing no obvious signs of tidal interaction or ongoing merger activity in this image. The observed color gradient from yellowish center to bluish outskirts hints at a declining star formation rate towards the galactic core, possibly due to quenching mechanisms. The majority of the galaxy's mass appears centrally located.
