The galaxy presents as an elliptical morphology, elongated in shape. A prominent central bulge exhibits a yellowish hue, suggesting a concentration of older stellar populations. The outer regions of the galaxy appear more diffuse and exhibit a bluer tint, potentially indicating the presence of younger stars or ongoing star formation. There are no obvious spiral arm structures or significant dust lanes visible in this image. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or recent merger events, although minor irregularities may be present upon closer inspection.
