The galaxy presents as an elliptical-type system, exhibiting a smooth, concentrated central bulge with a diffuse, less defined halo. The light distribution appears relatively uniform, with a gradual decrease in intensity from the core outwards. No distinct spiral arms or significant dust lanes are visible. The galaxy appears elongated in shape, with an axis ratio suggesting it is not viewed face-on. The color profile suggests an older stellar population. There is a hint of blue light at the edges of the galaxy. There is no strong evidence of ongoing major mergers or tidal disturbances in this system; however, there are some slight deviations from a perfectly smooth morphology.
