The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, potentially indicative of an older stellar population. Surrounding this core is a more diffuse region, displaying a subtle bluish tint that fades into the background. This outer region suggests the presence of a younger stellar population, possibly regions of ongoing, though not extremely vigorous, star formation. The overall shape is moderately elliptical, with a suggestion of being nearly circular. No significant tidal features, strong bars, or spiral arm structures are readily apparent. The overall impression is that of a relatively undisturbed, mature galaxy that has potentially undergone past mergers or accretion events.
