The galaxy presents an overall elliptical morphology with a bright, concentrated central bulge. The light profile suggests a relatively smooth distribution, though some subtle features are present. A faint disk-like structure seems to be present within the inner region. The central area exhibits a distinct ring-like formation surrounding the core of the galaxy. This ring shows some clumpy regions of star formation. The galaxy appears to be experiencing or has experienced a possible merger or tidal interaction event. Overall, there is a blue hue, indicating the presence of younger stellar populations.
