The galaxy appears as a relatively smooth, centrally concentrated object with a generally round morphology. The color gradient suggests a central bulge exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. There is a slight elongation, but the overall shape is not far from circular. Faint, diffuse extensions are possibly present around the main body, suggesting the presence of a tenuous halo or tidal features. The lack of clearly defined spiral arms or a prominent disk structure implies the possibility of an elliptical morphology or a lenticular galaxy seen from an angle that obscures any disk features. There's a subtle clumping of light in the central region, which could be a bright nucleus or concentrated star formation activity. The outer regions show a faint bluer light, suggesting younger stars are beginning to form there. 
