The galaxy presents as an elliptical form with a bright, concentrated central bulge. The bulge exhibits a high surface brightness, suggesting a dense population of stars, potentially an older stellar population. Surrounding the bulge is a fainter, more diffuse disk. The disk appears relatively smooth with a hint of a spiral arm structure. This suggests that it may be a spiral galaxy but is rather smooth compared to traditional spiral galaxies. The overall color of the galaxy suggests a mix of stellar populations, with the bluer colors hinting at the presence of recent star formation, especially within the disk region. There seems to be only minor disturbances within the galaxy. It appears mostly undisturbed.
