This galaxy exhibits a morphology suggestive of a system undergoing a merger or interaction. The overall form appears disturbed, deviating from a regular elliptical or spiral structure. There is an apparent pair of bright, somewhat diffuse nuclei, potentially indicating the presence of two distinct galactic centers nearing coalescence. These nuclei are embedded within a fainter, extended halo of stellar material. The light distribution is relatively smooth, though irregularities and asymmetries suggest tidal distortions. There is some evidence of faint tidal tails or bridges extending away from the main body of the galaxy, indicative of gravitational interactions. Color gradients are subtle, with a generally redder hue, hinting at an older stellar population and potentially lower ongoing star formation activity within the primary bodies. The system overall seems to be transitioning into a more homogenous elliptical-like structure.
