The galaxy presents as a disk-shaped system, tilted at an oblique angle to our line of sight. There is a noticeable central bulge that appears moderately sized and exhibits a yellowish hue, suggesting a population of older stars. Faint spiral arm structures are possibly discernible, but not distinctly defined. The overall color of the galactic disk is a combination of blue and redder tones, potentially indicating a mix of stellar populations and ongoing star formation within the spiral arms, as well as regions of dust obscuration. A bar structure may be present, though not particularly prominent. There is no obvious evidence of major merger activity or significant tidal disturbances. The overall appearance is that of a relatively undisturbed spiral galaxy with a moderate degree of central concentration.
