The galaxy appears to be undergoing a significant interaction or merger. It presents a disturbed morphology, not easily classified by standard Hubble types. Two distinct luminous cores are visible, one exhibiting a more concentrated and yellowish-white appearance, possibly indicative of an older stellar population. The second core displays a bluer hue, suggesting more recent or ongoing star formation. These cores are embedded within a larger, fainter halo of diffuse light. Patches of bluer light are scattered within the diffuse halo, further suggesting regions of active star formation. The overall shape is irregular and asymmetric, indicating gravitational disruption likely caused by the ongoing interaction. There are tidal features suggestive of elongated structures extending outward, though these are faint and somewhat indistinct. The galaxy has an estimated redshift of around 0.10, indicating that it is a fairly distant object. Its absolute magnitude suggests it is a relatively luminous galaxy, despite the obvious disruption. Given the luminosity and color gradients within the diffuse halo, star formation appears to be occurring throughout the object.
