The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an elliptical morphology with a high degree of roundness. The color gradient suggests an older stellar population, with a reddish core transitioning to slightly bluer outer regions. There is no distinct disk structure or prominent spiral arms visible. No major merger events are apparent; however, there may be some minor disturbances in the galaxy's morphology. The lack of strong blue emission indicates a low star formation rate. Overall, the galaxy is consistent with being an early-type galaxy such as an elliptical.