The galaxy appears as a centrally concentrated object, exhibiting a predominantly smooth morphology. It has an overall elliptical or spheroidal shape, with a noticeable lack of spiral arm structures or distinct disk-like features. The light distribution suggests a relatively even stellar population throughout the galaxy's body, though the central region appears slightly brighter, indicating a higher density of stars or possibly an active galactic nucleus. There are no signs of major disturbances or ongoing mergers, suggesting it is a relatively settled system. A very slight elongation is apparent, hinting at a deviation from perfect circularity, but no clear tidal features or extended halos are observed in this imaging. The color index indicates a population consisting primarily of older stars. Overall, it presents the characteristics of a mature, early-type galaxy.
