The galaxy presents as a single, largely homogenous structure with a smooth light profile. Its morphology is consistent with an elliptical galaxy, exhibiting a predominantly spherical shape with no discernible spiral arms or bar features. The color appears yellowish-orange, suggesting an older stellar population and a relative lack of ongoing star formation. There is a slight concentration of light towards the galactic center, forming a discernible but gentle central bulge. The outer regions gradually fade, indicating a decreasing stellar density with increasing distance from the core. There are no obvious signs of tidal distortions or recent merger activity.
