The galaxy presents a centrally concentrated light profile, indicative of a significant bulge component. It appears relatively smooth in overall morphology, with no prominent spiral arm structure or bar visible in this image. The central region exhibits a yellowish-orange hue, suggesting an older stellar population or dust obscuration. Surrounding the core, there's a broader, fainter halo with a bluer tint, possibly indicating more recent star formation activity in the outer regions. There may be a minor disturbance occurring within this galaxy's structure, but it appears to not be experiencing a major merging event. Based on its light and shape, this galaxy is most likely an elliptical or lenticular galaxy.
