The galaxy presents an overall elliptical morphology, appearing largely smooth with a concentrated central bulge exhibiting a slightly reddish hue. The main body displays a gradual fading in intensity from the center outwards. There is potential evidence of a disk component, but it is not sharply defined. A possible companion object or tidal disturbance is observed nearby, with a relatively smaller size and increased bluer color, indicating a more recent episode of star formation. There is no obvious indication of strong spiral arm structure, dust lanes, or an active galactic nucleus from this observation. Overall, the galaxy appears to be a relatively evolved system.
