The galaxy presents an overall elliptical morphology, elongated with a cigar-shaped appearance. The central region exhibits a brighter, more concentrated luminosity, suggesting a dense core or bulge. The galaxy shows a relatively smooth light distribution without prominent spiral arm structures. The color gradients suggest possible variations in stellar populations, with a subtle color shift from the inner to outer regions. The galaxy appears to be moderately inclined relative to our line of sight, as indicated by its elongated shape. There are no obvious signs of major disturbances or mergers, indicating a relatively settled state, though minor interactions cannot be ruled out.
