The galaxy exhibits a morphology that suggests a system undergoing interaction or a recent merger. The primary body of the galaxy appears somewhat amorphous, lacking a clear spiral or elliptical structure. There are multiple bright knots or clumps of luminosity, implying regions of concentrated star formation or tidal features resulting from gravitational interactions. The overall color profile indicates a mix of stellar populations, with some regions exhibiting bluer hues suggestive of younger, hotter stars, and other regions displaying yellower or redder tones, indicative of older stellar populations. A faint, extended halo or tidal stream seems to be present around the main galactic body, further supporting the interaction or merger scenario. There may be two or three distinct centers of light. The galaxy has a substantial stellar mass, as implied by its overall brightness and size. Its star formation rate is elevated, though not extreme, relative to its mass, suggesting moderate ongoing activity.
