The galaxy presents a generally smooth morphology, appearing somewhat elliptical in shape. A concentration of light is observed at the center, suggesting a prominent bulge. The galaxy exhibits a color gradient, shifting from a yellowish-white core to a bluer hue in the outer regions. While the overall structure appears relatively undisturbed, there is a hint of asymmetry, which may be due to minor disturbances or interactions. The outer edges of the galaxy are diffuse and lack well-defined spiral arms, indicating a potentially older stellar population.
