The galaxy presents a generally smooth and elliptical morphology. A concentrated, bright central bulge dominates the structure, exhibiting a yellowish-orange hue suggestive of an older stellar population. Surrounding the core, a fainter, more diffuse halo extends outwards, displaying a subtle gradient in color, shifting towards slightly bluer tones. There is no clear evidence of spiral arms or strong dust lanes. Minor asymmetry is present, but not pronounced. The overall light distribution suggests a relatively evolved system, potentially an early-type galaxy. No signs of major merging events are apparent.
