The galaxy presents a largely smooth morphology, exhibiting a notable absence of distinct spiral arm structures. The galaxy is compact and elliptical in shape, with a moderate degree of roundness. The primary color is a yellow-orange hue, indicating the presence of an older stellar population. The overall light distribution appears relatively uniform, with a possible slight concentration toward the center. There are no clear signs of major disturbances or ongoing mergers. Marginal amounts of star formation appear to be ongoing.