The galaxy presents a largely smooth and elliptical morphology. It appears highly rounded, lacking any significant disk-like features or obvious spiral arms. The color profile indicates a redder hue, suggesting an older stellar population is dominant. There is no visual evidence of active star formation regions, such as blue star clusters or HII regions, nor is there any major disturbance or interactions with other galaxies visible. Faint, diffuse light extends outwards from the central region, gradually fading into the background sky. The galaxy appears relatively undisturbed and likely represents a more evolved system.
