The galaxy presents a morphology that is predominantly smooth, exhibiting an elliptical or lenticular shape, but with subtle features. The galaxy appears flattened in shape, suggesting a possible disk structure. It exhibits a concentration of light towards the center, indicative of a bright central bulge or nucleus. Color gradients are present, with a yellowish hue concentrated in the core region, potentially indicating an older stellar population. Fainter bluish tinges are noted in the outer regions, which may indicate the presence of younger stars or ongoing star formation, albeit at a relatively low rate. There is some possible evidence of minor tidal disturbances, like faint plume-like extensions, but these are subtle. Overall, the system displays a complex interplay between smooth, evolved structures and hints of more dynamic processes.
