The galaxy appears as a relatively smooth, elliptical-like structure. It is centrally concentrated with a diffuse outer halo. The light distribution suggests an older stellar population, with a redder color compared to younger, star-forming galaxies. There is a subtle color gradient observed, with the central regions appearing slightly more yellow/orange than the outer regions, which are more red. This could indicate variations in the stellar populations, with older, redder stars dominating the central region. The galaxy exhibits minimal signs of spiral arm structure or significant dust lanes. Overall the galaxy appears undisturbed.
