The galaxy presents a largely smooth and rounded morphology, exhibiting a dominant central bulge with a gradual decrease in luminosity towards the outer regions. There are no prominent spiral arms or distinct features visible, suggesting a possible classification as an elliptical galaxy. The color profile appears generally uniform, trending toward the redder end of the spectrum. The light emitted suggest an older stellar population. There is a minimal sign of any ongoing mergers or tidal disturbances, indicating it is a relatively relaxed and undisturbed system.
