The galaxy presents as a relatively smooth, elliptical form. It appears to be quite round, exhibiting a high degree of radial symmetry. The core region is noticeably brighter and displays a yellowish-orange hue, potentially indicative of an older stellar population. Moving outwards from the core, there's a gradual decrease in surface brightness. A subtle blueish-green halo surrounds the central region, suggesting the presence of a younger population of stars or regions of recent star formation, although they appear subdued. There is no evidence of spiral arms or a defined disk. Overall, the galaxy appears undisturbed, lacking any obvious signs of ongoing or recent merger activity. The light distribution is fairly even, with no significant knots or irregularities visible.
