The galaxy appears to be a relatively smooth, disk-like structure, although without distinct spiral arm features. The central bulge exhibits a pronounced concentration of light, transitioning outwards to a less concentrated, more diffuse disk. The color profile shifts from reddish hues in the core to more greenish-yellow colors in the surrounding regions, indicating a potential change in stellar populations, dust content, or star formation activity with increasing radius. There are suggestions of some minor asymmetry or disturbances in the outer regions of the disk, possibly indicating past or ongoing minor interactions. Overall, the galaxy's morphology points to a system somewhere between a classical elliptical and a fully formed spiral.
