The galaxy appears as a merging system or a single galaxy with a significant tidal disturbance. The primary component presents a relatively smooth morphology and a generally round shape, with a concentrated central region. It displays a yellowish color, suggesting an older stellar population and lower levels of ongoing star formation. A second component is adjacent to the primary galaxy, possibly indicating an interaction or merger event. This component appears bluer, which could indicate younger stars and a higher star formation rate. There is a clear absence of well-defined spiral arms or a prominent disk. Given the merging or disturbed features and the estimated mass, this galaxy is potentially undergoing significant dynamical evolution.
