This galaxy appears to be an elliptical galaxy, exhibiting a relatively smooth and rounded morphology. There is a dominant central bulge that is bright and concentrated, with a yellow-orange hue, suggesting an older stellar population. Fainter, diffuse light extends outwards from the core, indicating the presence of an extended stellar halo. No distinct spiral arms or dust lanes are discernible. The overall color suggests that star formation is either minimal or has ceased. There are no signs of any active galactic nuclei or signs of being disturbed by a merger.
