The galaxy presents as a relatively small, moderately bright object with an overall elliptical morphology. It exhibits a smooth, featureless structure, indicative of an early-type galaxy, likely an elliptical or lenticular type. The color profile suggests a stellar population with a mixture of old and young stars, transitioning from a blue hue in the center to a reddish hue toward the edges of the galaxy. There appears to be a slight flattening of the spheroid, suggesting possible rotational support. No distinct spiral arms or dust lanes are visible. There's a slight asymmetry in the light distribution, potentially indicating a minor disturbance or ongoing interaction. The absence of prominent star-forming regions points to a low current star formation rate within the galaxy.
