The galaxy appears to be a relatively compact object, exhibiting a flattened spheroidal shape. The color distribution suggests a dominant population of older stars, evidenced by the yellowish hue in its central region. The galaxy also shows a distinct blue region of star formation on the side. There is an overall smoothness to the galaxy's light distribution, suggesting a lack of prominent spiral arms or significant dust lanes. There is some indication of a minor disturbance in the shape, but overall it looks to be a relatively undisturbed system. Based on the galaxy's color and morphology, it likely has a significant stellar mass and a relatively low star formation rate.
