The galaxy presents as a moderately inclined spiral. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. Spiral arms are discernable, though somewhat ill-defined and flocculent rather than grand design. These arms display subtle color variations, hinting at regions of ongoing star formation, albeit at a seemingly low rate. There is some evidence of a possible weak bar structure bisecting the central bulge. The disk appears relatively smooth, lacking any major signs of recent mergers or tidal disturbances. The galaxy's overall structure seems relatively undisturbed and quiescent, indicative of a system evolving in isolation.
