The galaxy presents a relatively smooth, elliptical morphology when observed in the visible light spectrum. The central bulge is prominent, with a high concentration of older stellar populations, exhibiting a yellowish-red hue. A disk component appears to be present; this galaxy is likely a lenticular (S0) galaxy. It displays a slight flattening. No prominent spiral arm structures are discernible; it lacks bright star-forming regions. There is no strong evidence of any recent or ongoing major mergers, with only minor disturbances in the morphological structure. There is a high degree of axial symmetry. Overall, this galaxy appears relatively undisturbed and evolved.
