The galaxy presents a primarily smooth morphology. The light distribution is relatively even, with a concentration of intensity toward the center. There is a suggestion of a slight elongation or asymmetry in the overall shape, hinting at a possible disk-like structure or minor tidal interaction, but this is not definitively confirmed by visual inspection. The galaxy's color appears to be primarily blue, indicating the presence of younger, hotter stars. There is some evidence of structure, such as a potential bulge or ring feature, but the dominant impression is one of relative homogeneity.
