The galaxy presents as a singular, relatively smooth object. It appears elliptical or spheroidal in shape, displaying a concentrated central bulge that diminishes gradually toward the edges. The color profile exhibits a moderate gradient, transitioning from a yellowish core to a bluer periphery. This suggests a potential distribution of stellar populations, with older, redder stars concentrated in the center and younger, bluer stars at the outer regions. There are some minor disturbances, but nothing suggesting major mergers. The galaxy appears to be moderately rounded.
