This galaxy exhibits a morphology indicative of an ongoing or recent merger event. There appears to be a primary, more luminous component and at least one secondary component, suggesting gravitational interaction and possible tidal distortions. The galaxy shows a generally amorphous shape, lacking clear spiral arm structures. Color gradients suggest a mix of stellar populations with a concentration of younger, bluer stars, and the overall luminosity appears to be indicative of a fairly massive galaxy with moderate star formation.
