The object appears to be a relatively smooth elliptical galaxy, displaying a concentrated central bulge and a gradual decline in surface brightness moving outwards. The galaxy exhibits a generally circular morphology with a high degree of symmetry. The color profile indicates an evolved stellar population, appearing predominantly yellow and red, suggesting that it is likely composed primarily of older, cooler stars. There is no clear indication of spiral arms or significant dust lanes. There is no morphological evidence of on-going or recent merger events. The galaxy presents a quiescent appearance, consistent with a low rate of star formation.
