The galaxy appears as an elliptical structure with a smooth morphology. The galaxy exhibits a concentrated central bulge that gradually diffuses into a less defined halo. Its color profile indicates a relatively old stellar population, trending toward redder wavelengths. The elongation suggests it is not perfectly spherical but rather slightly cigar-shaped. There is a potential indication of a minor disturbance in its symmetry, although this is not clearly defined. The galaxy's integrated light suggests it is a luminous object with moderate star formation activity. Overall, this galaxy presents as a massive, relatively quiescent system.