The galaxy presents as a spiral, observed at an oblique angle relative to our line of sight. A prominent central bulge is visible, exhibiting a yellowish hue. The disk component appears well-defined, displaying a mix of bluish and whitish tones suggestive of a stellar population with varying ages. Faint spiral arm structures are discernible within the disk. These arms appear tightly wound. No obvious interactions with other galaxies or major disturbances in its morphology are apparent. Overall the galaxy exhibits a well ordered structure.
