The galaxy presents a concentrated, roughly elliptical morphology. A bright central bulge is evident, exhibiting a cyan hue suggestive of relatively young, hot stars or active galactic nucleus activity. Surrounding the core is a diffuse, less intense region exhibiting a mix of colors. A subtle disk structure appears to be present, although it is disturbed. Patches of redder material are observed along the edges, which might indicate regions of dust obscuration or older stellar populations. There is a slight irregular feature on one side of the galaxy, giving a minor disturbed appearance. The overall structure suggests a galaxy undergoing or having recently undergone some form of interaction or disturbance. 
