The galaxy appears to be an elliptical type, exhibiting a smooth, largely featureless morphology. Its shape is generally ovoid, trending toward a more rounded structure, rather than an elongated or highly flattened disk. The light distribution is concentrated towards the center, which displays a bright core, and gradually decreases towards the outer edges. There is a slight color gradient, appearing yellower at the center and transitioning to a slightly bluer hue at the edges, which may indicate subtle variations in stellar population and age within the galaxy. There is no apparent spiral structure, bar, or significant dust lane obscuration visible. Indications suggest no recent major merger events or significant tidal disturbances in its recent history. The galaxy shows overall a quiescent state of star formation activity.