The galaxy presents an overall elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region displays a bright, yellowish-white color, likely indicating an older stellar population.  There is a slight elongation or cigar shape. Subtle extensions can be observed away from the central bulge. Possible faint hint of a disk. There appears to be a very slight blue component visible in the outer regions, suggestive of some ongoing star formation, albeit at a low rate.  The overall structure appears relatively undisturbed, with no obvious signs of a major merger event, though a minor disturbance cannot be ruled out.
