This galaxy presents as an edge-on spiral with a pronounced central bulge. The bulge appears relatively smooth and concentrated, suggesting a significant population of older stars. A faint, extended disk is visible, oriented horizontally in the image. The disk exhibits a subtle dust lane obscuring the central region, indicating the presence of interstellar dust and gas. The outer regions of the disk appear somewhat diffuse, with hints of spiral structure although it is not clearly defined. There is no clear evidence of a major ongoing merger or significant tidal disturbance. The galaxy exhibits a warm color, leaning towards reddish-orange, possibly indicating a moderate amount of on-going star formation. There is a slight variation in brightness along the galactic disk with a slight amount of asymmetric distribution. The bulge appears slightly elliptical, and it blends smoothly into the disk.
