The galaxy presents as a fairly smooth, elliptical structure with a concentrated, bright central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or significant dust lanes. The galaxy exhibits a color gradient, appearing more yellow in the central region and slightly bluer towards the outer edges. This color variation suggests a possible difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars possibly present in the outskirts, though star formation appears to be largely suppressed throughout the galaxy overall. The galaxy shows a generally round shape, lacking any strong distortions or signs of ongoing major mergers, though a small nearby galaxy suggests there may be some minor interactions occuring.
