The galaxy presents an overall elliptical morphology, with a smooth, centrally concentrated light profile. The core exhibits a yellowish hue, suggestive of an older stellar population. Moving outwards from the core, a subtle transition to bluer colors is observed, possibly indicating regions of more recent, albeit limited, star formation. No distinct spiral arm structures or strong dust lanes are apparent. The galaxy exhibits a moderate degree of roundness and does not appear to be undergoing any major merging events or significant tidal disturbances, although there is possibly a very minor disturbance.
