The galaxy presents a generally smooth morphology, with a concentrated central bulge. The light distribution appears centrally dominated, with a gradual decrease in intensity outward from the core. The apparent shape is somewhere between round and elliptical. There is a very slight indication of a possible disk structure, although it is not prominent. No clear signs of strong tidal disturbances or ongoing major mergers are detected, although a possible minor disturbance is not ruled out. Color gradients suggest a slightly bluer outer region than the core, potentially indicating ongoing, but relatively low, levels of star formation. The colors appear reddest in the center, with the overall color profile indicating a relatively mature stellar population.
