The galaxy presents a somewhat elongated, elliptical morphology, though it is closer to a circular appearance. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density. Moving outward from the core, the luminosity gradually diminishes, but faint structures are present. Subtle, irregular features can be observed within the galaxy's structure. A hint of spiral arm structure is visible, but these features are not distinct and could be interpreted as general irregularities within the galactic disc. The colour profile suggests an older stellar population, particularly in the core, but possible star forming regions are present. The colour variations are quite subtle, indicating a relatively homogeneous stellar population throughout the galaxy. The morphology suggests that this galaxy may be a transitioning galaxy, with the appearance of a smooth elliptical galaxy, but with some indications of spiral arms.
