The galaxy presents as a single, relatively smooth object with a slightly elliptical morphology. Its light profile is dominated by a central bulge region that exhibits a yellowish-orange hue, suggesting an older stellar population. Surrounding the bulge, there is a faint, extended halo of light that is primarily green, possibly indicative of ongoing star formation. There is a subtle hint of asymmetry or disturbance, potentially suggesting a minor interaction or past merger event, but the overall structure appears largely undisturbed. 
