The galaxy presents as an edge-on spiral type. A prominent central bulge is visible, appearing smooth and elongated along the galactic plane. The bulge exhibits a rounded morphology, lacking distinct boxy features. The disk is oriented nearly perfectly edge-on relative to our line of sight. There is no visible evidence of ongoing major merging activity or significant tidal disturbances. A slight asymmetry in the disk's outer regions might suggest minor gravitational interactions or internal processes. The color distribution shows a somewhat bluer tint in the disk region, indicating the possibility of younger stellar populations, while the bulge displays a yellower hue, likely comprised of older, redder stars. Light from the galaxy indicates a moderate level of star formation. The smooth, elongated appearance contributes to the impression of a well-established, relatively undisturbed galactic structure.
