The galaxy presents as an elongated, disk-shaped structure, oriented nearly edge-on relative to our line of sight. A prominent central bulge is visible, exhibiting a concentrated luminosity gradient, indicative of a high stellar density. The bulge appears approximately rounded in shape. The disk component exhibits a relatively smooth texture. There is a slight indication of color variation across the galaxy, the bulge appearing more yellowish, whereas there may be subtle bluish hints in the disk, possibly suggestive of ongoing star formation. There is no strong evidence of tidal features, major mergers, or significant disturbances in the galactic morphology based on this image.
