This galaxy presents as a generally smooth and rounded object. The core region appears relatively bright and concentrated, exhibiting a yellowish hue, potentially indicative of an older stellar population. There is little evidence of distinct spiral arms or a prominent disk structure, but a subtle extension is visible on the lower side of the galaxy, with bluer colors suggestive of some star formation. The galaxy shows no signs of major tidal disturbances or ongoing mergers, appearing as a single, relatively undisturbed system. The intermediate roundness suggests a morphology between perfectly spherical and elongated.
