The galaxy presents an elliptical morphology, exhibiting a smooth and concentrated light profile. Its color index suggests a population dominated by older stars, resulting in a yellowish hue. The overall shape leans towards a flattened spheroid, with a suggestion of deviation from perfect roundness. There are subtle indications of minor disturbances in its structure, but the galaxy generally appears as a relaxed system. Evidence of ongoing star formation is minimal based on its color and morphology. The galaxy does not show any signs of a major merger.
