This galaxy presents as a relatively elongated, disk-shaped structure viewed nearly edge-on. A central bulge is prominent, exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk itself appears mottled, displaying a color gradient from the core outward. Fainter, bluer light is seen along the edges of the disk, hinting at ongoing star formation in these regions. There is no evidence of any major mergers or tidal disturbances. There appears to be some faint, diffuse material extending slightly beyond the main galactic plane on either side of the galaxy, possibly representing a halo or extended stellar disk. The disk is relatively smooth.
