The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated luminosity, suggesting a higher density of stars or potentially an active galactic nucleus, though further spectral analysis would be needed to confirm the latter. The galaxy appears to be slightly elongated, rather than perfectly spherical, with its light gradually fading toward the outer edges. A faint, bluish halo surrounds the galaxy, which could indicate the presence of younger stars, or more likely, ongoing star formation, particularly in the outer regions. However, the overall morphology points towards it being a well-matured, evolved galaxy. There appears to be a very slight amount of disturbance in the morphology, and thus could be a hint of a minor interaction with another galaxy. 
