The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses outward into a fainter, more extended halo. The galaxy is generally round in appearance, displaying only subtle deviations from perfect circularity. No distinct spiral arms or prominent dust lanes are discernible in this image. There is no evidence of ongoing major mergers or significant tidal distortions, though subtle disturbances may be present. Overall, the galaxy appears to be a relatively evolved system with characteristics consistent with a low star formation rate. The galaxy's color profile suggests a population of older stars, contributing to its overall appearance.
