The galaxy presents as a relatively compact and bright object. The morphology is predominantly smooth in appearance, indicating a possible elliptical or lenticular classification. There may be evidence of faint, diffuse features suggestive of a disk, but this is subtle. The galaxy exhibits a fairly round shape. The galaxy appears undisturbed, lacking any prominent signs of tidal tails or distortions that would indicate a recent or ongoing merger event. The color profile suggests a moderate amount of star formation is likely ongoing. 
