The galaxy presents a complex morphology, appearing as a merging system. A primary component exhibits a smooth, elliptical-like structure. Adjacent to this main body is a secondary, more compact component showing a higher concentration of light, potentially indicating a younger stellar population or increased star formation activity. There appears to be gravitational interaction occurring, with evidence of tidal tails or bridges extending between the two merging galaxies. The overall color suggests a mix of stellar populations. The primary galaxy shows more red and orange light, indicative of older stars, while the secondary galaxy has bluer colors, implying younger, hotter stars. There is a third possible component.
