The galaxy presents a generally smooth morphology, with a dominant spheroidal component. Its overall shape appears elongated, approaching a cigar-like appearance. A central concentration of light is evident, surrounded by a more diffuse halo. There is a slight indication of a disk feature, but its contribution is minor. No significant merger activity or major disturbances are observed; however, there might be minor disturbances. Color gradients show a more yellow/orange hue towards the galactic center, which suggests a population of older stars. The outer regions of the galaxy exhibit bluer tinges, indicating the presence of younger stellar populations, but star formation appears to be relatively quiescent.
