This galaxy presents as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The light distribution suggests a dominant population of older stars, giving it a redder hue in comparison to bluer, star-forming galaxies. There's a possible slight distortion or tidal feature visible, hinting at a past or ongoing interaction with another galaxy. Overall, the morphology points towards a galaxy undergoing a period of quiescence, with a low rate of star formation activity.
