The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its color appears relatively uniform across the structure, exhibiting a yellowish-white hue that suggests an older stellar population. No distinct spiral arms or features suggestive of active star formation are clearly visible. The overall shape approximates an elliptical form, appearing somewhat flattened, lacking a defined disk-like structure. There is some evidence of minor asymmetry in the outer regions, but no evidence of active merging events. The galaxy exhibits a moderate degree of luminosity, indicative of a substantial stellar mass.
