The galaxy presents a generally smooth, rounded morphology, appearing largely featureless at this resolution. The light distribution suggests a spheroid-dominated system with minimal evidence of a prominent disk structure. There is a concentration of brighter, bluer light towards the central region with a gradual decrease in intensity towards the outer edges. The overall color gradient indicates a redder, and thus likely older stellar population in the outskirts. The galaxy appears undisturbed with no obvious signs of recent or ongoing major merger events. Based on morphology alone, it is consistent with being an elliptical galaxy.
