The galaxy appears to be an elliptical galaxy, characterized by a relatively smooth and featureless morphology. Its light profile is centrally concentrated, showing a gradual decrease in luminosity from the core outwards. The core region exhibits a yellowish hue, potentially indicating an older stellar population. There is an absence of spiral arm structures or prominent dust lanes. Overall the galaxy appears to be fairly compact with hints of disturbance, possibly due to a minor merger event in its past.