The galaxy presents an elliptical morphology, exhibiting a smooth light distribution with no apparent spiral arms or bar structure. The core region of the galaxy is significantly brighter and more concentrated, suggesting a higher density of stars towards the galactic center. The galaxy exhibits a color gradient, with the core appearing more yellowish-white and the outer regions displaying a slightly bluer hue. This could indicate a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars more prevalent in the outer regions. There is some subtle asymmetry in the outer regions, suggesting possible minor tidal disturbance or a recent, smaller merger event, but generally it looks like the galaxy is not strongly interacting with another object. 
