The galaxy presents an overall elliptical morphology. It appears relatively smooth in texture, with a central bulge that is noticeably brighter and more concentrated than the surrounding regions. This core exhibits a yellowish hue, suggesting an older stellar population.

Fainter, diffuse light extends outward from the central bulge, forming a somewhat elongated shape. Hints of bluer light are observed in the outer regions, possibly indicating the presence of younger, hotter stars. The overall color gradient suggests radial variation in stellar populations within the galaxy. There may be some minor disturbances in its morphology, but the bulk of the galaxy is undisturbed. There is no major disturbance, feature, or disk present. It is not undergoing any significant merging activity. 
