The galaxy presents a somewhat elliptical morphology, appearing largely smooth and centralized in its light distribution. There is a concentration of yellowish light toward the galaxy's core, suggesting an older stellar population is dominant in this region. Fainter, bluer light extends outward from the center, particularly on one side, which could indicate ongoing or recent star formation in that area. The overall structure lacks prominent spiral arms or a well-defined disk, and it appears relatively undisturbed, showing minimal signs of interaction with other galaxies.
