The galaxy appears to be a relatively smooth, elliptical or lenticular type, with a high degree of central concentration. It exhibits a prominent, bright nucleus that graduates into a less luminous, diffuse halo. There's minimal evidence of spiral arm structure or significant dust lanes. The galaxy presents a slightly elongated, but generally rounded shape, showing hints of being somewhat oblate. There might be a very slight disturbance in its morphology, such as a minor asymmetry, but overall it is a relatively undisturbed system. The galaxy has a dominant yellow to orange color in its core, which is typical of older stellar populations, grading into bluish tones in the surrounding region. Overall, the galaxy presents as a moderately massive system with modest levels of ongoing star formation activity.
