The galaxy presents as a largely smooth, elliptical-type object, with minimal discernible disk features. The morphology appears well-rounded. There is a dominant central bulge that exhibits a yellowish hue, suggesting an older stellar population and lower star formation activity. The outer regions of the galaxy exhibit a bluer tint compared to the central bulge, implying the presence of some younger, hotter stars. No significant signs of tidal disturbances or ongoing mergers are immediately apparent from the image. The galaxy appears relatively isolated in its environment.
