The galaxy presents a generally elliptical morphology. The light distribution appears relatively smooth and concentrated towards the center. There is no prominent spiral arm structure visible, suggesting a lack of significant ongoing star formation in a disk. The central region exhibits a brighter, more compact core, potentially indicating the presence of an active galactic nucleus or a region of higher stellar density. Faint color variations can be discerned, trending towards redder hues in the central bulge and potentially bluer tones in the outer regions, hinting at variations in stellar populations. The overall appearance is consistent with a galaxy in an intermediate stage of evolution, possibly transitioning from a spiral to an elliptical form. There is some evidence of minor gravitational disturbance.