The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology suggests a significant fraction of its light comes from an older stellar population. The object exhibits an elliptical or lenticular shape, with a generally round appearance rather than a highly elongated form. Some minor disturbances or irregularities may be present in the galaxy's structure, but they are not prominent enough to suggest a major ongoing merger event. There is no clear spiral arm structure visible. The galaxy displays a moderate color gradient, transitioning from a slightly more yellow/orange hue in the central region to a somewhat bluer tint toward its outer edges. This might suggest some ongoing, but not extreme, star formation activity.
