This galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction or merger. The central region displays a bright, concentrated core, potentially indicative of an active galactic nucleus or a dense stellar population. Extending outwards from the core, there are faint, diffuse tidal features, appearing as streams or tails of stellar material. The overall color gradient indicates a mix of stellar populations, with the central region appearing yellower, perhaps due to older stars, while the outer regions show bluer hues, suggesting more recent star formation. The disk appears to be viewed edge-on. The observed features support classification as a merging system with evidence of both established and newly formed stellar populations.
