The galaxy presents a largely smooth, elliptical morphology. Its central region exhibits a high concentration of light, appearing yellowish, suggesting an older stellar population. The light gradually diffuses outwards, showing hints of reddish hues in the intermediate regions, possibly indicating a mix of older and intermediate-age stars. The galaxy lacks any prominent spiral arm structures or distinct dust lanes. There are no clear signs of tidal tails or significant morphological disturbances, although subtle asymmetries cannot be entirely ruled out given the image resolution. The outer regions of the galaxy fade gently into the background, indicating a smooth transition in stellar density. Overall, the galaxy appears to be a relatively quiescent system with a dominant bulge component.
