The galaxy exhibits a generally smooth morphology. The light distribution appears concentrated towards the center, suggesting a prominent bulge. The overall shape appears to be slightly elongated, neither perfectly spherical nor highly flattened. There may be some minor asymmetry present in the outer regions, possibly indicative of a past or ongoing interaction, though no major disturbances or merging features are clearly visible. Color gradients are subtle, with a slightly bluer hue observed in the central region compared to the outskirts, although the galaxy has little or no emission in the Z band. This may suggest a population of younger, hotter stars present in the galaxy's core, indicating recent star formation.
