The galaxy presents as a relatively smooth, elliptical-like structure with a notable central bulge that dominates its overall light profile. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars within that region. Moving outwards from the center, the luminosity gradually decreases, forming a more diffuse halo. The galaxy appears elongated, with a cigar-like shape, but without any obvious spiral arm structures or dust lanes. There are minor irregularities in the outer regions, hinting at possible gravitational interactions or disturbances. The blue color suggests the presence of some younger stellar populations, but the dominant light is more consistent with older stars.
