The galaxy appears as a centrally concentrated object, elongated in shape, with a relatively smooth overall texture. The central region presents a bright, yellowish-white hue, which gradually fades towards the outer edges. The color profile suggests a dominant older stellar population in the core, consistent with less active star formation. The lack of distinct spiral arms or a defined disk structure indicates that it is likely an elliptical galaxy. The smooth and featureless morphology suggest the galaxy is undisturbed, and is not currently undergoing a major merging event. A small amount of bluer regions may indicate low levels of on-going star formation at the outskirts. Overall, the observed characteristics align with those expected of a passively evolving galaxy.
