The galaxy presents a largely smooth morphology, appearing elliptical in shape. The central region exhibits a concentrated luminosity, shifting towards redder wavelengths, suggestive of an older stellar population. The outer regions display a gradual decrease in luminosity and a shift towards bluer wavelengths, potentially indicating areas of more recent star formation. There is no clear evidence of spiral arm structures or a distinct galactic disk. The galaxy appears relatively isolated with no obvious signs of major interaction or merging events, though a slight asymmetry could suggest minor gravitational disturbance. Overall, the galaxy seems to be a massive system with ongoing, albeit moderate, star formation activity.
