The galaxy presents a generally smooth appearance, with some indication of a disk structure. There is a slightly elongated form, but overall the light distribution suggests a relatively round object. The central region exhibits a concentration of light, implying a bulge or core. Moving outwards from the core, the color shifts slightly, suggesting a change in the stellar population, with more yellow and red stars further from the center. Faint features, potentially indicative of spiral arms or tidal disturbances, can be very vaguely discerned. Overall, the galaxy seems to be relatively undisturbed.
