The galaxy appears as a concentrated, elliptical-shaped system. It exhibits a smooth, featureless morphology, with no prominent spiral arms or distinct dust lanes visible. The galaxy's light profile is centrally concentrated, exhibiting a gradual decrease in luminosity moving outward from the core, but is fairly round. Color gradients are subtle, with a slightly redder hue towards the center and a slightly bluer hue towards its outer regions. There is no evidence of significant tidal disturbances or interactions with neighboring galaxies. The galaxy displays an overall red color, possibly indicating an older stellar population and lower star formation activity. 
