The galaxy presents as a generally elliptical form. It exhibits a bright, concentrated central bulge, suggesting a high density of stars in its core. The galaxy's overall color appears to be yellowish-white, potentially indicating an older stellar population with fewer young, massive stars. There is evidence of a faint, diffuse disk or halo surrounding the central bulge. The disk does not show any distinct spiral arm structures, but the overall morphology suggests some form of ordered rotation. There are slight asymmetrical features present in the outer regions of the disk, potentially indicating a minor gravitational disturbance or recent interaction with another galaxy. Based on the overall appearance, the galaxy seems to be relatively evolved with a low rate of star formation.
