The galaxy presents as an elliptical-like structure with a smooth, concentrated light profile. There is a bright central bulge that appears nearly spherical, indicative of an older stellar population. The color gradient suggests a redder core that transitions to bluer hues in the outer regions. There are no obvious spiral arms or dust lanes visible in the image. The outer edges of the galaxy are diffuse, fading gradually into the background sky, revealing a lack of sharp boundaries. There may be a faint halo surrounding the main body of the galaxy. There are no signs of any major merging activity, but possibly very minor disturbances. The structure is overall very regular, and the round shape is indicative of it being an early type galaxy.
