The galaxy presents an elliptical morphology, appearing relatively smooth and lacking distinct spiral arm structures. Its overall shape is somewhat elongated, displaying a cigar-like appearance rather than a perfectly circular form. The core exhibits a brighter, more concentrated luminosity, suggesting a higher density of stars in the central region. A gradual decrease in brightness is observed towards the outer edges of the galaxy. The galaxy displays a color gradient, appearing yellowish-white at the center and transitioning to a slightly redder hue towards the outskirts. There is no obvious evidence of ongoing major merger activity. The galaxy does not have any noticeable substructure.
