The galaxy appears as a centrally concentrated object with a generally smooth morphology. It presents an elliptical or spheroidal shape, appearing mostly round, with a slight deviation from perfect circularity. No obvious spiral arm structures or significant disk features are discernible in the image. The light is dominated by a yellowish hue in the central region, suggesting a population of older stars, with slightly bluer outskirts, possibly indicating some ongoing, albeit low-level, star formation activity in its outer regions. There is no strong evidence of major disturbances or mergers in the image, although some minor asymmetry might hint at a past interaction or internal dynamics. The galaxy appears relatively isolated, without any immediately obvious major companion galaxies in the immediate vicinity.
