The galaxy presents a generally amorphous morphology, with a central, bright core. The core appears relatively smooth. Surrounding the core is a diffuse halo of bluer light, which extends unevenly from the central region. There is no strong visual evidence of spiral arms or a defined disk structure. The bluer hue of the surrounding halo suggests the presence of younger stellar populations or ongoing star formation. There is some potential evidence of minor tidal disturbances or interactions, with slight asymmetry to the overall structure.
