The galaxy presents a morphology that appears largely smooth and centrally concentrated, with a subtle decrease in luminosity towards the outer regions. It is roughly elliptical. The primary color is a somewhat reddish-yellow hue, indicating a likely population of older stars and a limited amount of on-going star formation. There is a slight blue tint present in a bright region, hinting at a population of younger stars in this area. There is no clear evidence of spiral arm structure or a prominent central bar. There may be a very minor asymmetry or disturbance, but generally, it appears relatively undisturbed, and not undergoing any major merging events.
