The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be primarily elliptical in shape, deviating slightly from a perfect circle, with a hint of elongation along one axis. The light distribution is characterized by a bright, yellow core, suggesting a population of older stars dominating the central region. A subtle color gradient is observed, transitioning from the yellow core to slightly redder hues in the outer regions. There may be a very faint, diffuse disk, but this is difficult to ascertain given the limited resolution and smoothness of the galaxy's overall light profile. No distinct spiral arms or significant dust lanes are visible. The overall structure suggests that the galaxy is likely a relatively evolved system with a high degree of stellar population homogeneity.
