The galaxy presents as an elliptical-like system with possible merger activity or significant tidal interactions. The core exhibits a smooth, concentrated luminosity profile, with a Sersic index greater than 3, suggesting a bulge-dominated morphology. The galaxy's shape appears somewhat elongated, exhibiting an ellipticity of approximately 0.5. The observed color gradient indicates a relatively red galaxy, implying an older stellar population. The presence of dual nuclei is suggestive of either an ongoing galactic merger or a close interaction, which could explain the disturbed morphology and potentially elevated star formation rates. The galaxy's overall color is indicative of a quiescent system with minimal recent star formation.
