The galaxy appears to be an elliptical galaxy, with a notable lack of spiral arm structure. It exhibits a smooth, diffuse light distribution that declines gradually from the center. The core is bright and concentrated, with an apparent elongation along a northeast-southwest axis. Faint extensions or a very diffuse halo seem to surround the main body of the galaxy but are hard to resolve, suggesting an aged stellar population, or perhaps a Sersic profile with a high 'n' value where light drops off slower than other galaxies. There is a slight color gradient visible, with the central regions appearing somewhat yellower than the outer parts, which may suggest a difference in the stellar population or dust content. The general color indicates the presence of older stars.
