The galaxy appears to be a roughly elliptical system, exhibiting a concentrated central bulge that transitions smoothly into a fainter, more diffuse halo. The color profile suggests an older stellar population, with a yellow-orange hue dominating the central regions. There is a slight hint of bluer colors in the outer regions which might suggest some ongoing star formation, though the galaxy overall appears quiescent. The galaxy also seems to show signs of morphological disturbance, perhaps due to a past or ongoing minor interaction with another galaxy. The overall morphology suggests a relatively massive system.
