The galaxy presents a smooth, elliptical morphology. There is a concentrated central bulge that is bright and appears yellow-white in color, suggesting an older stellar population. The overall shape is elongated, with a high degree of symmetry around the major axis. The galaxy exhibits a gradual decrease in brightness from the core outwards, with a faint, diffuse halo surrounding the central region. There is little evidence of spiral arms or distinct features. The overall color suggests relatively low levels of ongoing star formation. There is a very slight indication of minor disturbance in the galaxy shape, but no significant signs of a major merger. 
