The galaxy presents an overall elliptical morphology with a predominantly smooth texture. There is a possible, faint disk-like structure. The galaxy's light distribution appears concentrated towards the center, suggesting a prominent bulge.

Color gradients within the galaxy are noticeable. The central region exhibits a yellowish-white hue, potentially indicating an older stellar population. A secondary concentration of light towards the right of the image shows a reddish tint. To the bottom of the galaxy there is a bluish hue. These color variations could be due to differences in stellar populations, dust content, or star formation activity. 

There is slight evidence of disturbance in the galaxy's morphology. These features may be indicative of tidal interactions with another galaxy, although the main body appears relatively undisturbed. It is possible that the galaxy has undergone a minor merger event in the past.
