The galaxy appears as a relatively bright, ellipsoidal structure with a smooth, featureless morphology. There is a slight elongation, but it is generally round. Its color suggests a mature stellar population, with a redder hue indicating older, less active star formation. There is no visual evidence of spiral arms or a prominent central bar. The galaxy's smooth appearance suggests it may be an elliptical galaxy or a lenticular galaxy seen face-on. There might be minor disturbances potentially suggestive of a previous or ongoing interaction, however, this could be the product of resolution quality. The galaxy does not seem to be actively merging with any other prominent objects, although faint disturbances cannot be ruled out. The light distribution is centrally concentrated and seems to be mostly uniform.
