The galaxy presents as a moderately luminous object with an overall elliptical morphology. The central region exhibits a significantly higher surface brightness, appearing quite smooth and concentrated, suggesting a prominent bulge component. Extending outwards from the core, the galaxy displays a less defined, fainter halo or envelope. There is evidence of a possible tidal tail or minor disturbance along the top of the galaxy, however, given the image quality, the galaxy could also be merging. The color profile reveals a redder core, indicating an older stellar population, while the outer regions appear slightly bluer, potentially indicative of more recent star formation. The overall smoothness of the galaxy suggests that it is a relatively evolved system.
