This galaxy appears to be a relatively smooth, elliptical galaxy with a dominant central bulge. The light distribution is concentrated towards the center, indicating an older stellar population. There is a slight elongation, deviating from a perfect sphere. No prominent spiral arms or dust lanes are visible, suggesting a lack of significant ongoing star formation. There is a hint of a diffuse halo surrounding the main body of the galaxy, which could be comprised of older, dispersed stars. Overall, the galaxy seems to be an evolved system that is not undergoing any major mergers or disturbances.
