The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. There is a notable central bulge region that transitions to a fainter, more diffuse halo extending outwards. The general shape appears to be close to round. Subtle indications suggest possible minor disturbances or asymmetries in the outer regions, though not conclusive. The color profile indicates a stronger presence in the green portion of the spectrum. No spiral arm structures or significant dust lanes are observed.