The galaxy presents a primarily smooth morphology, exhibiting a centrally concentrated bulge with a gradual decrease in luminosity towards the outer regions. Its overall shape appears elliptical, deviating slightly from a perfect circle, tending more towards an intermediate elliptical form. The color profile suggests an older stellar population, particularly within the central bulge, which is characterized by a yellowish-orange hue. This may imply a lower rate of on-going star formation, supported by the relatively red color. There are faint hints of a disk-like structure or arm features, but the smoothness of the galaxy dominates, indicating a more evolved system. No significant signs of recent merger activity or major disturbances are readily apparent in the image, though a subtle asymmetry could suggest minor past interactions or internal dynamics.
