The galaxy presents as a spiral structure, although partially obscured by its moderate inclination relative to our line of sight. The disk component is evident. Spiral arms are discernible, exhibiting a winding morphology. The central bulge dominates the overall luminosity, indicating a significant concentration of older stellar populations. The galaxy appears barred. The bulge appears moderately sized, indicating some mass, but not a primary component of the light. There are no obvious signs of interaction or ongoing mergers with other galaxies; its structure appears relatively undisturbed, suggesting recent dynamical stability. The galaxy's color indicates ongoing star formation, although moderate.
