The galaxy exhibits a roughly circular morphology with a bright, concentrated core. There appears to be a degree of irregularity or disturbance in its overall structure. It presents a diffuse, extended halo surrounding the central region. Evidence suggests potential tidal features or disrupted arms, indicative of a gravitational interaction. The color profile suggests a mix of stellar populations. The bluer hue in the outer regions might be due to younger, hotter stars, while the central region seems slightly redder, possibly indicating older stars or dust obscuration. Overall, the galaxy appears to be undergoing or have recently undergone a merging event, evident from its irregular features.
