The galaxy presents a generally smooth, elliptical morphology. It displays a slight elongation, deviating marginally from a perfectly circular form. The light distribution appears relatively homogenous, with a concentration towards the center, suggesting a higher density of stars in the galactic nucleus. Color gradients are subtle, with a hint of reddish hues concentrated in the central region. The overall color index indicates a population of older stars, potentially suggesting a relatively low ongoing star formation rate. There is some indication of minor tidal disturbance, but the galaxy largely appears undisturbed.
