The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is generally round and slightly elongated. There is a noticeable color gradient with a bluer central region and redder outer regions. This color variation suggests a difference in stellar populations, with possible younger, hotter stars concentrated towards the galactic center. There's a slight visual asymmetry, with a subtle hint of distortion along one axis, suggesting a possible interaction or past minor merger event. The overall impression is of a galaxy undergoing a relatively quiescent period of star formation, but not completely inactive. The galaxy does not seem to have a pronounced disk structure, but the light distribution has a smooth profile.