The galaxy presents as a concentrated, elliptical-like structure with a high degree of central light concentration. The core region exhibits a yellow-orange hue, suggestive of an older stellar population. There is a subtle extension of light surrounding the core that is slightly green in appearance, possibly hinting at a small amount of ongoing star formation. The galaxy appears relatively smooth with no obvious spiral arms or distinct features. It shows a high degree of rotational symmetry. There is a slightly smaller object nearby to its left which may be a companion galaxy.
