The galaxy presents as a centrally concentrated object, with an overall elliptical morphology. A relatively smooth appearance dominates the central bulge, which exhibits a yellowish-white color, possibly indicative of an older stellar population. Some asymmetry can be observed, and there appears to be a slight disruption to the morphology, suggesting a recent or ongoing interaction or merger. Patches of redder emission are visible, which could be a sign of star forming regions. Based on this analysis, the galaxy may be an elliptical galaxy undergoing or having recently undergone a merging event, and it exhibits relatively low levels of star formation activity for its mass.
