The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile. It shows a slight elongation, deviating minimally from a perfectly circular shape. There is a bright, concentrated core with a yellowish hue, suggesting a population of older stars. Moving outwards from the core, the galaxy fades into a less luminous halo. The lack of clearly defined spiral arms or dust lanes suggests a relatively quiescent star formation history. There may be a very slight minor disturbance to the morphology, however no significant merger activity is apparent. 
