The galaxy presents an overall smooth, elliptical morphology. Its central bulge appears bright and concentrated, exhibiting a yellowish hue suggesting an older stellar population. Moving outward from the center, the color shifts to a slightly greenish tint. This could indicate the presence of a younger population of stars. The galaxy's shape is closer to being an oval than a pure circle, but not extremely elongated. There are no obviously signs of spiral arm structure. There is no clear evidence of a major ongoing merger with another galaxy, however, there may be subtle distortions in the outer regions of the galaxy indicative of a minor disturbance, possibly an interaction with a smaller companion. 
