The galaxy appears as a centrally concentrated, elliptical-like structure exhibiting a smooth morphology. Its color profile suggests an older stellar population, potentially dominated by redder giant stars. The galaxy presents a roughly circular projected shape, with some deviation from perfect roundness. There is a possibility of minor interaction or disturbance suggested by slight asymmetries. The light distribution indicates a non-negligible degree of central concentration. The estimated absolute magnitudes suggest that this galaxy is a luminous object. Logarithmic star formation rate indicates that it is not a very active galaxy.
