The galaxy presents an overall elliptical morphology, appearing largely smooth and relatively featureless. The central region exhibits a concentrated luminosity profile, suggesting a prominent galactic nucleus. The color gradient transitions from a yellowish-white core to bluer hues in the outer regions, implying a possible decline in stellar age and/or an increase in star formation activity in the outer disk. There is a subtle indication of a disk component with a slight flattening of the galaxy’s shape along one axis. It does not appear to be undergoing any major merging events, but there is a slight asymmetry to it, which may suggest minor gravitational disturbances. Based on its color, brightness, and size, it appears to be a moderately sized galaxy.
