The galaxy exhibits a predominantly smooth morphology, suggesting an elliptical or lenticular classification. It presents with a bright, concentrated core that gradually diffuses outwards. The overall color profile indicates an evolved stellar population, with a dominance of older, redder stars. A slight elongation or tidal tail is potentially visible, which could indicate a past or ongoing interaction with another galaxy. This structure is characterized by a less intense red hue than the central region. The lack of distinct spiral arms or prominent dust lanes reinforces the interpretation of a relatively quiescent, early-type galaxy, although a minor merger cannot be ruled out.
