The galaxy appears to be an elliptical, with a generally smooth morphology, though not perfectly spherical, appearing slightly elongated. The central region exhibits a high concentration of light, suggesting an older stellar population. The overall color gradient indicates that the central bulge is yellower, becoming slightly bluer in the outer regions; this may indicate the presence of some younger stars further from the galaxy's center. There is no clear evidence of spiral arms or a prominent disk structure. There are some slight irregularities on the outer edges of the galaxy, but it is otherwise undisturbed.
