The galaxy presents as a slightly inclined spiral, though the arm structure is not sharply defined. A bright, concentrated central bulge dominates the visual appearance, exhibiting a yellowish hue. Fainter, bluer regions are observed in the disk, hinting at younger stellar populations and ongoing star formation. The overall shape appears relatively smooth, indicating a possible lack of recent major merger events, though some minor disturbances may be present within the disk structure. The galaxy's light profile suggests it is a massive galaxy, with considerable luminosity. It is likely undergoing a modest rate of star formation, considering its color and the potential presence of stellar populations.
