The galaxy presents as a relatively smooth, elliptical morphology. The central bulge appears dominant, exhibiting a bright, concentrated luminosity with a slightly orange-red hue. The outer regions display a gradual decrease in surface brightness, with a less distinct, more diffuse structure. There is a slight hint of distortion in the outer regions, but no clear evidence of spiral arms, a bar, or a major ongoing merger. The galaxy appears to be generally isolated, with only subtle indications of minor disturbances in its structure. The shape is somewhat intermediate, neither perfectly round nor significantly elongated. The color gradient suggests older stellar populations are more centrally concentrated. Overall, the galaxy appears to be a massive, relatively evolved system.
