The galaxy presents an overall elliptical morphology, with a relatively smooth light distribution. The central region exhibits a noticeable concentration of light, appearing brighter than the surrounding areas. A distinct, somewhat flattened, disk-like structure is visible within the central region. There is evidence of potential disturbances or interactions, possibly indicating ongoing or past mergers. The colors suggest a mix of stellar populations, with the central region displaying a bluer hue and the outer regions appearing redder, possibly due to differential dust extinction or variations in star formation rates. Faint tidal features or plumes may be present extending away from the main body of the galaxy.
