The galaxy presents as a relatively smooth, centrally concentrated object. The light profile suggests an elliptical morphology or a lenticular galaxy viewed at a low inclination angle. The central region displays a significantly brighter, more concentrated emission, transitioning to a gradual fading towards the outer regions. There is some evidence of a slight disturbance or tidal feature on the right side. A notable feature is the object located near the center, which could be indicative of a minor merger. The general color of the galaxy appears to be red, suggesting an older stellar population. No distinct spiral arms are visible.
