The galaxy presents a largely featureless, smooth appearance. The overall shape appears generally elliptical, trending toward a slightly more rounded form, though the resolution is not high enough to precisely define its ellipticity. The light distribution shows a strong concentration towards the center, exhibiting a prominent central bulge that gradually diffuses outwards. The color profile suggests a dominant population of older stars, contributing to the yellowish-orange hue of the galaxy, particularly in the core region. Very faint hints of bluer light are seen in the outer regions, perhaps suggesting some low-level ongoing star formation, but it is not prominent. There is no obvious indication of spiral arm structure or strong dust lanes. There are no signs of any major interactions or mergers.
