This galaxy presents a predominantly disk-like morphology. The central bulge is moderately sized and displays a concentrated luminosity, surrounded by a fainter and bluer disk. I observe a prominent bar feature spanning a significant portion of the galaxy's central region. Faint spiral arm structures appear loosely wound and extend outwards from the bar's ends. The arms show evidence of ongoing star formation. The galaxy appears relatively isolated. The overall color suggests the presence of both older stellar populations in the bulge and younger, bluer stars in the disk.
