The galaxy presents a diffuse, roughly elliptical morphology. A bright, concentrated core region is visible, surrounded by a fainter, more extended halo. Within the core, there is a suggestion of complex structures. The color profile appears relatively uniform, though slightly bluer in the innermost regions, hinting at the presence of younger stellar populations or active star formation. There is some indication of minor structural distortions extending outwards from the main body of the galaxy, possibly tidal tails or other features indicative of gravitational interaction. The outer regions exhibit a granular texture, which may represent unresolved stellar populations or dust clouds. Although it appears largely non-interacting at first glance, subtle disturbances exist.
