The galaxy appears as a centrally concentrated object with a largely smooth morphology. It displays a round shape with a slightly elliptical profile, indicating a lack of significant rotational support. The primary color is a yellowish-white, which could suggest an older stellar population. There is no discernible spiral arm structure or bar. There is no clear evidence of major mergers or tidal disturbances, although minor interactions cannot be ruled out. The overall structure suggests a relatively evolved system with ongoing but not vigorous star formation.
