The galaxy presents as a largely featureless, smooth elliptical. It exhibits a high degree of circularity, appearing almost perfectly round. The galaxy's luminosity profile suggests a centrally concentrated morphology. There are no apparent spiral arms, bar structures, or other disk-like features discernable within the limitations of this image. The color profile suggests a dominant population of older stars, indicated by the slightly redder hue in the central region. There is no evidence of any major ongoing merging events or tidal distortions. A minor asymmetry may be present in the outer halo, but this could be attributed to image noise. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
