The galaxy presents a predominantly smooth morphology, exhibiting a relatively featureless structure. The light distribution appears concentrated towards the center, suggesting a prominent bulge component. The galaxy appears moderately rounded in shape and shows no signs of major tidal disturbances or ongoing mergers, though a faint hint of minor asymmetry cannot be ruled out. The color profile appears relatively uniform, with a slight reddening towards the central region. The overall appearance indicates a system where star formation is ongoing, albeit at a moderate rate, with a stellar mass that is characteristic of dwarf galaxies.
