The galaxy presents an elliptical morphology with a smooth light distribution, exhibiting a concentrated central bulge. The axial ratio suggests the galaxy is viewed at a moderate inclination. Color gradients indicate that the central regions are redder than the outer regions, which could be indicative of differing stellar populations or dust distribution. There is no clear evidence of spiral arms or a prominent disk structure. The overall color suggests a relatively evolved stellar population and low star formation activity. Minor irregularities in the outer regions suggest possible minor disturbances or interactions.
