The galaxy presents as a somewhat amorphous, centrally concentrated object. It exhibits a moderate degree of smoothness in its overall light distribution, with no readily apparent spiral arm structures or prominent dust lanes. The shape is generally roundish, with a slight elongation. The core region shows a concentration of light that appears more yellow/orange. Overall, the galaxy exhibits a redder color profile, which can be an indicator of an older stellar population or significant dust extinction within the galaxy. There is no visually detected ongoing interaction with another object, but some internal disturbances cannot be ruled out. The galaxy's morphology suggests a galaxy with a large mass, but a low star formation rate.
