The galaxy presents a largely smooth morphology with a bright, concentrated central region. The overall shape is approximately round, exhibiting a slight elongation. There is a subtle suggestion of a disk or spiral structure. The galaxy's color profile appears redder toward the center, suggestive of an older stellar population, with a hint of bluer colors in the outer regions, potentially indicating ongoing star formation. There is no obvious evidence of major merging activity or significant tidal disturbances. The galaxy's luminosity is relatively high, indicative of a substantial stellar mass.
