The galaxy presents a generally smooth, elliptical morphology. The light distribution suggests a concentration towards the center, with a bright core. The galaxy appears elongated, exhibiting an intermediate shape between round and cigar-shaped. There's no obvious evidence of spiral arm structures or a distinct disk component. Faint color variations can be observed throughout the galaxy, which could indicate different stellar populations. No major merger events or significant disturbances are apparent in the galaxy's structure, though there are possibly slight asymmetries.
