The galaxy appears to be a relatively smooth, elliptical-like structure. The central region displays a concentrated, bright, and yellowish hue, possibly indicating an older stellar population. Moving outwards from the center, the light gradually fades and transitions to a slightly bluer color, suggesting the presence of some younger, hotter stars within a disk-like structure. There's a faint hint of asymmetry or subtle disturbance in the outer regions, but it generally maintains an elliptical form. No strong signs of a major merger are apparent. The galaxy's morphology leans towards a quiescent system with a potential for mild ongoing star formation.
