The galaxy presents a somewhat elliptical morphology, appearing oblong rather than perfectly spherical. The central region exhibits a concentrated, yellowish-white hue, suggestive of an older stellar population dominating this area. Fainter, bluer light extends outwards from the core, indicating the presence of younger stars or regions of active star formation, although these features appear less pronounced. There appears to be little evidence of defined spiral arms or a prominent disk structure; instead, the galaxy appears mostly smooth and relatively undisturbed. Overall, the galaxy's light distribution suggests a system in a relatively late stage of its evolution, possibly transitioning to a more quiescent state. There is no strong indication of a major ongoing merger or significant tidal disturbances.
