The galaxy presents a flattened elliptical morphology, appearing largely smooth and featureless. The central region exhibits a distinct reddish hue, indicative of an older stellar population or dust obscuration. Moving outward from the core, the color transitions to a bluer tint, potentially signifying younger stars in the outer regions. There is a subtle suggestion of a disk-like structure, though it appears quite diffuse rather than sharply defined. The overall shape suggests a galaxy that is more spheroid than spiral, with a hint of possible elongation along a preferred axis. No signs of significant tidal disturbances or ongoing mergers are readily apparent.
