The galaxy presents an elliptical morphology, exhibiting a relatively smooth and concentrated light distribution. The core region appears to be a bright, centralized bulge. The light profile indicates a high degree of roundness, with a slight deviation toward an intermediate elliptical shape. There is a slight color gradient, from a bluer core region to redder outer regions. No obvious spiral arms, dust lanes, or other disk features are discernible. There is a hint of a slight disturbance on one end of the galaxy. Overall, the galaxy appears undisturbed, and not currently undergoing major merging activity. The structure of the galaxy indicates a well-formed, and largely undisturbed system.
