The galaxy appears to be a luminous, centrally concentrated object, exhibiting a smooth, elliptical morphology. The dominant color is a yellowish-orange hue, suggesting an older stellar population with relatively low levels of ongoing star formation. A smaller, somewhat distorted, and less luminous object appears closely associated, potentially indicating a minor interaction or disturbance. This smaller object exhibits a bluer color profile compared to the main galaxy, possibly containing younger, hotter stars. Overall, the system presents as an elliptical galaxy, potentially undergoing or having undergone a minor merger event.
