The galaxy presents as a centrally concentrated object with an overall elliptical morphology. The core exhibits a high degree of luminosity, appearing nearly spherical. The surrounding galactic structure appears relatively smooth, with no prominent spiral arm features or distinct dust lanes visible. A slight bluing is evident around the central bulge, possibly indicating ongoing star formation. There are no obvious signs of major galactic mergers or tidal disturbances, but a minor asymmetry could imply a subtle interaction or internal rearrangement. The object has an approximate effective radius of 3.5 kpc, which is likely an underestimation due to image blurring. Based on its morphology, the galaxy is likely relatively massive and demonstrates low levels of star formation.
