The galaxy appears as a moderately bright, diffuse object with an overall elliptical morphology. There is a discernible central bulge that is brighter and more concentrated than the surrounding regions. The color of the central bulge appears slightly redder compared to the outer regions of the galaxy. The outer regions display a bluer hue.  There are some indications of subtle, asymmetrical features or disturbances, possibly faint tidal tails or warped structures, suggesting a potential history of gravitational interaction or minor merger event.  The overall appearance suggests a system with a moderate amount of ongoing star formation, primarily located in its outer regions.
