The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth morphology without prominent spiral arms or a well-defined disk structure. The overall shape is somewhat elongated but predominantly elliptical, with a degree of disturbance and a possible merger event. The central region exhibits a bright core, indicating a concentration of older stellar populations. The galaxy displays a color gradient, appearing bluer in its outer regions, possibly indicating pockets of younger stars. The apparent merging behavior suggests a complex gravitational interaction with another galaxy, potentially in an early stage of coalescing into a single, larger system.
