This galaxy appears to be a relatively smooth, elliptical galaxy with a centrally concentrated luminosity profile. The galaxy's shape is elongated, exhibiting an intermediate axial ratio, and lacks any obvious signs of spiral arm structures or significant dust lanes. The central bulge is quite bright and yellow in color, suggesting an older stellar population. Fainter, more diffuse light extends outwards from the core. There is a slight color gradient from the center to the outer regions, with the core appearing yellower and the outer parts exhibiting hints of bluer light, likely tracing regions of sparse, younger stars. There does not appear to be evidence of major recent or ongoing mergers. The galaxy's smooth morphology suggests it is a mature system that has largely completed its merging history.
