This galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile. The galaxy's overall shape appears largely spherical, with minimal visible deviation from roundness. 

Color gradients are apparent. The central region displays a yellowish-orange hue, potentially indicative of an older stellar population. Progressing outward, the galaxy exhibits a slight decrease in color temperature, transitioning toward redder hues in the outer regions, suggesting the potential for ongoing, albeit diminished, star formation in the galactic periphery.

Evidence suggests a potential merging event or tidal interaction. The presence of some features may indicate disturbances within the galaxy's structure.
