The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a gradual decrease in luminosity from the core outwards, indicating a diffused distribution of stars. The galaxy appears nearly circular, with a slight elongation. The color profile indicates the presence of older stellar populations, particularly within the central region, suggested by the yellowish-white hue. There's little evidence of distinct spiral arms or significant dust lanes. The galaxy exhibits a smooth, featureless morphology, indicative of an evolved system.
