The galaxy presents as an elliptical or lenticular-type morphology. Its light distribution appears smooth and centrally concentrated, lacking distinct spiral arm structures. The galaxy exhibits a moderate degree of roundness, tending toward an intermediate shape rather than a perfectly circular or elongated form. There are no obvious signs of major mergers or significant tidal disturbances affecting its overall structure, although minor disturbances cannot be ruled out. The object's color suggests a population of relatively old stars, indicative of a lower rate of ongoing star formation.
