The galaxy appears to be a spiral galaxy, observed at a significant angle to our line of sight, presenting a somewhat edge-on view. The central bulge exhibits a bright, yellowish hue, suggesting a population of older stars. The spiral arms are visible, albeit somewhat faint and tightly wound. These arms display a bluer tint, likely indicative of ongoing star formation and the presence of younger, hotter stars. There's evidence of dust lanes along the inner edges of the spiral arms, partially obscuring the light from behind. Overall, the galaxy exhibits a well-defined, symmetrical structure, with no obvious signs of major tidal disturbances or interactions with other galaxies. The galaxy is of substantial size.