The galaxy presents as a slightly elongated, lenticular structure. It appears to be relatively smooth and featureless, lacking any distinct spiral arms or prominent dust lanes. The central bulge is noticeable and exhibits a concentrated, bright yellowish-orange hue, suggesting an older stellar population. Moving outward from the center, the light gradually fades, transitioning into a more diffuse halo. There is a hint of asymmetry in the outer regions, potentially indicating minor gravitational interaction or past merger events. Overall, the galaxy's morphology is consistent with an elliptical or S0 type, displaying a largely quiescent nature with likely low ongoing star formation activity.
