The galaxy exhibits a roughly elliptical morphology, appearing somewhat rounded. It shows a prominent central bulge with a high concentration of light, exhibiting a yellow-orange hue which likely indicates an older stellar population. The outer regions display a fainter, more diffuse structure. There appears to be some evidence of disk-like features, and there may be subtle hints of spiral arm structure in the faint outer regions, but this is not definitive. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances. It's a relatively smooth and well-defined system.
