The observed galaxy presents as a spiral galaxy, exhibiting a generally face-on orientation relative to our line of sight. The galaxy possesses a prominent central bulge, characterized by a concentrated luminosity gradient. The spiral arms appear well-defined. The arms display a tightly wound morphology emanating from the central bulge. The galaxy shows faint and extended disk, with no clear signs of ongoing major merger events. There are no prominent dust lanes observed. The galaxy does not appear to be a barred spiral.
