The galaxy presents a largely smooth, elliptical morphology. There is a bright, concentrated central bulge that dominates the galaxy's light profile. There are no readily apparent spiral arm structures or dust lanes visible in this image, which is consistent with an early-type classification. The overall color appears relatively uniform with a slight reddening towards the central regions. The galaxy does not appear to be undergoing any major merging events. The round shape suggests a minimal rotational component. The relative lack of blue light and the presence of reddening indicates an older stellar population.
