The galaxy presents a largely smooth and concentrated appearance, suggesting an elliptical morphology. The central region exhibits a bright, yellowish hue, indicative of an older stellar population, potentially dominated by red giant stars. Moving outwards, the light gradually fades and becomes slightly redder, forming an extended halo. There is no clear evidence of spiral arms or a distinct disk structure. Minor asymmetrical light distribution could indicate slight disturbances from past interactions, though the galaxy appears largely undisturbed. The lack of blue color suggests a very low star formation rate within the galaxy. The galaxy is moderately sized.
