The galaxy presents a generally smooth, elliptical morphology. It exhibits a slight elongation, appearing somewhere between round and cigar-shaped, but closer to round. A dominant central bulge is visible, contributing significantly to the overall luminosity. The color gradient suggests a population of older stars, exhibiting a redder hue at the core which fades further away from the core into a yellower hue. There is a subtle hint of a disk structure, but the overall smoothness suggests it is not a spiral galaxy. There is no obvious sign of strong tidal interactions or major disturbances, although a slight asymmetry could indicate minor gravitational interaction with smaller, unseen neighbors.
