The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology with a high degree of roundness. A subtle color gradient is noticeable, transitioning from a yellow-white hue in the core to a more blue-green tinge towards the outer regions. This might indicate the presence of a younger stellar population in the galaxy's periphery. There's no visually apparent spiral structure, bar, or tidal features suggesting recent major mergers. However, some minor irregularity could hint at a minor disturbance or past interaction. The galaxy appears to be a substantial object, with a mass likely greater than the average dwarf galaxy. Overall, the observed characteristics suggest a galaxy dominated by an older stellar population, with a low rate of star formation.
