The galaxy appears to be a relatively smooth, somewhat asymmetrical object. There is evidence of a disk structure, with some indication of features, potentially faint spiral arms, or tidal disturbances. The galaxy exhibits a concentration of light toward its center, but without a particularly bright or well-defined core. The overall color profile suggests a mixture of stellar populations, with bluer hues indicating younger, hotter stars and redder hues potentially indicating older, cooler stars. The galaxy shows only minor signs of any mergers, or disturbances.
