The galaxy presents a largely elliptical morphology, exhibiting a smooth light distribution. The core region is characterized by high luminosity, fading gradually toward the outer edges. The galaxy shows an overall round shape, with a slight departure from perfect circularity. There is some evidence of minor structural irregularity. There appear to be no signs of prominent spiral arms or a distinct galactic disk. No major merger events are visible, however there may be some minor signs of a previous merger in the form of disturbed light distribution. Colors of the galaxy suggest a population of older stars with less ongoing star formation.
