The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. It exhibits a bright, nearly circular core, which gradually fades into a diffuse halo. There is a slight color gradient, with the core appearing more yellow-white and the outer regions exhibiting a slightly redder hue. No distinct spiral arms or prominent dust lanes are visible. The overall morphology suggests an evolved system, possibly a spheroidal galaxy lacking significant ongoing star formation. There is a possible slight disturbance of its symmetry, suggesting a minor interaction has occurred or is occurring. The system has an estimated diameter of around 4 kpc. The galaxy's integrated light suggests a redder stellar population, consistent with older stars.
