The galaxy presents a generally smooth appearance with a slightly elongated, elliptical morphology. A distinct central bulge is visible, appearing more concentrated and possessing a yellowish hue, suggesting an older stellar population. The outer regions exhibit a fainter, more diffuse quality. There is a subtle color gradient apparent, with bluer tones extending towards the edges, potentially indicating regions of recent or ongoing star formation. There are no prominent spiral arm structures or significant dust lane features detectable in this image. Overall, the galaxy appears relatively undisturbed, without obvious signs of major merger activity.
