The galaxy presents an elliptical morphology. The light distribution is centrally concentrated, exhibiting a smooth profile with no obvious spiral arm structures or prominent dust lanes. The color gradient suggests a population of older stars dominating the central region, indicated by its yellowish-orange hue. The outer regions appear slightly bluer, potentially indicating a younger stellar population or ongoing, albeit subdued, star formation. There appears to be a subtle disk component. Overall, the galaxy shows no strong evidence of recent major merger activity, though minor disturbances cannot be ruled out based on the image alone.
