The galaxy presents a generally smooth appearance, exhibiting a subtle disk-like structure. The central region displays a concentrated, bright core, indicative of a bulge. The galaxy is elongated, with a cigar-shaped morphology. There's a hint of a spiral structure, though it is not well-defined. The color gradient suggests older stellar populations dominate, particularly towards the center, while bluer regions are less pronounced. No obvious signs of major merging events or significant tidal disturbances are apparent. The galaxy appears relatively isolated.
