The galaxy presents a predominantly elliptical morphology with a smooth, diffuse structure. Its central region exhibits a pronounced concentration of light, appearing yellowish-orange, possibly indicating an older stellar population. The outer regions gradually fade into a fainter, bluish halo. A subtle disk-like feature may be present within the overall elliptical shape, evidenced by a slightly flattened appearance. There are hints of minor disturbances or features within the galaxy, though they are not overtly pronounced. The overall color suggests moderate ongoing star formation with a significant population of older stars.
