The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. Its core exhibits a distinct yellowish hue, suggesting an older stellar population dominating the central regions, indicative of minimal recent star formation. 

A faint, reddish extension is observed emanating from the central region, hinting at possible tidal disturbances or a minor merging event. The overall roundness of the galaxy is apparent, however some form of feature is observable, indicating that the object may not be fully relaxed. The estimated mass is significant, placing this galaxy within the category of massive systems. The specific star formation rate is low.
