The galaxy exhibits a generally smooth morphology, appearing as a somewhat elliptical, disk-like structure. The central region shows a brighter, more concentrated luminosity, suggesting the presence of a galactic bulge. The galaxy's color gradient shifts from a yellow-white core to a redder and slightly dimmer outer region. There is minimal evidence of spiral arm structures or significant dust lanes. No signs of any current merging events or major disturbances are apparent. The galaxy appears to be in a relatively settled state, possibly in the process of transitioning from a spiral to elliptical type galaxy, though still exhibiting some disky features.
