The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, indicating a prominent nucleus or bulge. The light distribution gradually fades from the center outwards, suggesting a decreasing stellar density. There might be subtle signs of disturbance, such as minor asymmetries in the outer regions of the galaxy, potentially caused by past interactions, although these are not particularly apparent. There isn't a clear disk structure, spiral arms, or prominent dust lanes. The overall color index suggests a mix of stellar populations.