The galaxy presents as a moderately bright, elliptical form. Its core region exhibits a concentrated, orange hue, suggesting an older stellar population. This core is surrounded by a less intense, more diffuse halo exhibiting a slight greenish tint. The elongation of the galaxy indicates a non-spherical structure, closer to an intermediate elliptical form. There's no evident spiral arm structure or prominent dust lanes. Minor asymmetry is noticeable, but no clear signs of tidal disturbances or merging activity are apparent. Overall, it appears to be a relatively undisturbed, evolved galaxy.
