This galaxy exhibits an elliptical morphology, appearing smooth and featureless. Its shape is elongated, with a clear major and minor axis. The central region displays a concentrated luminosity, indicative of a bulge potentially dominated by older stellar populations. The outer regions of the galaxy fade gradually into the background, suggesting a diffuse stellar halo. The color profile appears generally redder in the central regions, transitioning to slightly bluer hues in the outer edges, possibly indicating ongoing star formation in the galactic disk. There's no evidence of strong spiral arm structure or significant dust lanes. The overall structure seems undisturbed, without obvious signs of a major merger event.