The galaxy presents an overall elliptical morphology, appearing largely smooth and featureless in this imaging. It exhibits a concentrated central bulge that appears roughly spherical, with a gradual decrease in luminosity extending outwards. There is some slight asymmetry in its overall shape, possibly indicative of a past or ongoing minor interaction with another galaxy. The color is generally redder, suggesting an older stellar population and diminished star formation activity. There is a hint of a faint disk surrounding the central bulge. No prominent dust lanes or spiral arm structures are discernible.
