This galaxy exhibits a disturbed morphology, potentially indicative of a past or ongoing merger event. The central region appears relatively compact, although poorly resolved. Distinct tidal features such as faint tails or streams cannot be clearly discerned. The galaxy displays a predominantly blue hue, implying a relatively young stellar population and active star formation, concentrated in some regions. The galaxy's overall color index suggests a moderate redshift. However, the galaxy lacks a well-defined spiral arm structure. Evidences show the galaxy is potentially undergoing some sort of merging process. High resolution imaging and spectroscopic follow-up would be beneficial to determine more characteristics and properties of this galaxy.
