The galaxy presents an elliptical morphology, appearing somewhat elongated in shape. Its light distribution is centrally concentrated, with a smooth, diffuse halo extending outwards. The central region exhibits a yellowish hue, suggesting an older stellar population. A faint, reddish concentration is observed at one edge of the halo, possibly indicating a region of recent star formation or a merging event. Overall, the galaxy appears relatively undisturbed, lacking prominent spiral arms or other distinct structural features.
