The galaxy presents as a centrally concentrated object with a generally smooth appearance. It exhibits a somewhat elliptical morphology, appearing nearly round but with a slight elongation. There's a bright central region that fades gradually into the outer areas. Faint blue hues are present, particularly towards the core, which likely indicates the presence of younger stellar populations and ongoing star formation. Some subtle disturbances or irregularities are observed in the outer regions, although these are not prominent enough to suggest a major ongoing merger. Overall, the galaxy appears relatively undisturbed, with a dominant spheroidal component.
