The galaxy appears as a relatively luminous and compact object. Its morphology suggests a spheroidal shape, displaying a smooth light distribution, though there is some evidence of disturbed features within the structure. The central region exhibits a high degree of roundness, with the outer regions possibly showing a subtle deviation from a perfectly circular form. There is an indication of a potential interaction or merger event, signified by irregularities in the galaxy's form and light profile. Overall, the galaxy displays characteristics somewhere between an elliptical and a disturbed morphology, suggesting a dynamic system undergoing some form of structural transformation.
