The galaxy presents a morphology suggesting an ongoing or recent merger event. The overall structure is irregular, exhibiting a disturbed appearance rather than a well-defined spiral or elliptical form. Multiple luminous cores are apparent, potentially indicative of the nuclei of the merging galaxies. The color profile suggests a mixed stellar population, with yellowish hues dominating the central regions, possibly indicating older stars. The galaxy appears relatively smooth in areas, yet hints of disturbed features are present, with some elongation and fuzziness. The system shows signs of moderate tidal interactions, disrupting the original galactic structures. The galaxy is relatively compact, with a moderate size of approximately 6 kiloparsecs across its widest extent. Overall, the galaxy’s features imply significant dynamical activity, likely fueled by the interaction and eventual coalescence of multiple galaxies.
