This galaxy presents a generally smooth and elliptical morphology. The central region exhibits a brighter, more concentrated luminosity profile, suggesting a higher density of stars in the galactic nucleus or the presence of an active galactic nucleus. The overall color is relatively uniform, with a subtle gradient towards bluer hues in the outer regions, possibly indicating the presence of younger stellar populations or ongoing star formation at the periphery. There is no evidence of prominent spiral arms or a well-defined disk structure. The galaxy appears largely undisturbed, lacking significant tidal features or signs of recent major mergers. However, there might be minor asymmetrical features that imply minor disturbances of some sort. The generally smooth appearance points toward this galaxy being a more evolved system.
