The galaxy presents as a largely featureless object with a concentrated central bulge, exhibiting a smooth, elliptical morphology. Its overall shape appears quite round, with a slight elongation that is barely discernible. The color profile suggests an older stellar population, with a yellowish hue dominating the central region, possibly indicating a greater abundance of evolved stars and reduced ongoing star formation. There is no clear evidence of spiral arms or a disk-like structure, nor any signs of active galactic nuclei activity or recent merger events. The galaxy appears relatively isolated and undisturbed.
