The galaxy presents a morphology suggestive of an elliptical or lenticular classification. The light profile appears largely smooth and centrally concentrated, exhibiting a notable lack of distinct spiral arm structures. A subtle disk-like structure may be present, but it is not prominently featured. The galaxy's shape is neither perfectly spherical nor markedly elongated, indicating it is most likely an elliptical galaxy that isn't perfectly circular. There are no major disturbances observed, there also appears to be little to no interaction with nearby galaxies. The color gradient suggests an older stellar population dominating the galaxy, contributing to a subdued star formation rate.
