The galaxy presents as a lenticular or edge-on spiral morphology. It exhibits a bright, concentrated central bulge that appears relatively smooth in texture. There is a faint disk component visible extending outward from the bulge, wider than the bulge, but not as wide as it is long. One side of the disk appears less defined. A faint hint of spiral structure is possible on the brighter edge. Subtle color variations suggest some ongoing star formation, predominantly located within the disk region. The galaxy's overall shape is elongated, indicating an inclination to our line of sight. There is some mild asymmetry in the galaxy's overall structure, particularly in the disk region, suggesting a possible past interaction or merger event, or internal dynamics. The galaxy's luminosity suggests a substantial mass, indicative of a mature system.
