The galaxy presents as a flattened, elongated structure with a significantly brighter central bulge. Its overall color is a yellowish-white, suggesting an older stellar population concentrated in the core. The outer regions show a bluer hue, possibly indicating the presence of younger, hotter stars within a faint disk or spiral arm structures, though these features are not sharply defined. The galaxy's morphology leans toward an elliptical shape, but with a disk component, making it a possible lenticular galaxy observed at an angle. The galaxy's apparent smooth texture suggests that if spiral arms exist, they are tightly wound. There is little evidence of active star formation in the central region, based on the lack of strong blue emissions there. The elongation suggests a degree of rotation and a relatively low bulge-to-disk ratio.