The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is largely elliptical, exhibiting a high degree of roundness. The light is concentrated towards the core, which displays a yellowish hue suggesting an older stellar population. There is a slight blue tint in the outskirts of the galaxy, this suggests some ongoing star formation, albeit less intense than in actively star-forming galaxies. No major distortions or tidal features are apparent, indicating that the galaxy is likely not undergoing any significant merger events. 
