The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated towards the center, which exhibits a yellow-orange hue, potentially indicating an older stellar population. Progressing outward, the galaxy transitions to a more diffuse, blue-green halo. This could signify a younger, star-forming population existing in the galactic outskirts, or a scattering effect. The overall shape is nearly round, with only a slight elongation. No prominent spiral arms or bar structures are discernible. There is no evidence of major merging activity. A faint distortion might be present in the outer reaches, potentially from a prior interaction, though it is likely minor.
