The galaxy presents as an elongated, disk-like structure, oriented approximately vertically in the image frame. There is a noticeable central bulge, characterized by a bright, yellowish-orange hue, suggesting a population of older stars. The disk component appears somewhat less defined, displaying a more diffuse and bluer coloration, potentially indicating regions of ongoing star formation. While the galaxy appears largely undisturbed, there is a subtle asymmetry to the disk, possibly hinting at a past or ongoing minor interaction. Overall, the galaxy appears as a relatively massive, star-forming system at a considerable distance.
