The galaxy presents as an edge-on spiral, its disk oriented approximately horizontally in the frame. A prominent central bulge dominates the galaxy's luminosity, appearing with a yellowish hue, suggesting a population of older stars. This central bulge exhibits a relatively smooth profile. The disk component is visibly thinner and extends outwards from the bulge, displaying a faint bluish tint, potentially indicating regions of ongoing star formation within younger stellar populations. The disk shows evidence of a dust lane obscuring some of the light from the central bulge, appearing as a dark band running along the galactic plane. There are no obvious signs of recent major merger activity or tidal disturbances in the galaxy's morphology. The galaxy has a well-defined, although slightly diffuse, edge.
