This galaxy exhibits a complex morphology with features suggestive of tidal interactions or a recent merger event. The main body appears diffuse, lacking a well-defined nucleus or spiral arm structure. There is an irregular distribution of light, with brighter and dimmer regions scattered throughout. A faint, extended halo is visible, primarily green and blue. Faint tail-like features may be present, extending outwards from the main body. Areas of disturbed morphology are evident, suggesting gravitational interactions or ongoing star formation activity. The lack of distinct spiral structure and presence of irregularities indicate that it may be either an irregular galaxy or an elliptical galaxy experiencing a merger event. Further spectroscopic and photometric analysis is required to determine the nature of this galaxy.
