The galaxy presents as a somewhat elliptical structure. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars or possibly an active galactic nucleus. The color of the central bulge leans towards yellow/red, which indicates an older stellar population. The outer regions of the galaxy exhibit a fainter and slightly bluer hue relative to the core. This may indicate some degree of ongoing star formation. There is very slight indication of disruption in the lower right quadrant, suggesting that some gravitational interactions may be occurring. 
