The galaxy presents a largely smooth, elliptical morphology. Its light is concentrated towards the center, exhibiting a bright core that gradually diffuses outwards. There are no apparent spiral arms or distinct features suggestive of ongoing major mergers. The overall color profile appears to be relatively uniform, with subtle gradations in hue, perhaps indicating a lack of significant dust lanes or intense, localized star-forming regions. The general roundness and lack of sharp edges suggest a relatively relaxed dynamical state. There is very faint disturbance in the outer regions. The smooth appearance points toward a population of older stars, but some younger populations are likely indicated by the blue hues. The galaxy shows a small amount of star formation. 
