The galaxy presents a generally smooth morphology, with a high degree of roundness. There's a central concentration of light that fades into a diffuse halo. No strong spiral arm structures or bars are apparent. There is a slight blueish hue to the edges. Some minor disturbances or faint features may be present, but the overall impression is that of a relatively undisturbed system. No signs of major mergers or tidal tails are visible, which supports its classification as a non-merging system. The color profile suggests the presence of older stellar populations, with a possible contribution from ongoing star formation in the outer regions. The galaxy exhibits a moderate redshift, indicating a substantial distance. The size is relatively compact.
