The galaxy presents an elliptical morphology, appearing largely smooth in texture without prominent spiral arms or a defined disk structure. There is a slight elongation, but it primarily appears round. Its color profile indicates a greater concentration of older stellar populations with an absence of strong blue light indicative of ongoing, vigorous star formation. There is a central region with a more concentrated brightness, likely indicating the presence of a substantial galactic bulge. Evidence of interactions or mergers is minimal; the overall structure seems relatively undisturbed, with a possible faint disturbance.