The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a generally smooth and concentrated light distribution. The central region is noticeably brighter and more yellow, suggesting an older stellar population. The outer regions are less defined and appear slightly bluer, potentially indicating a small degree of recent star formation. The overall shape is roughly circular. No distinct spiral arms or bar structures are evident. There are no signs of major mergers or significant tidal disturbances.
