The galaxy presents as a moderately bright, disk-shaped structure with a prominent central bulge. Its overall color appears to be primarily bluish-white, suggesting a significant population of younger, hotter stars. The shape is elongated, indicating an inclined disk, observed at an angle relative to our line of sight. There is evidence of faint, diffuse spiral arm structure extending from the central bulge. The galaxy appears relatively undisturbed, though subtle irregularities in the outer disk may hint at minor interactions. The galaxy displays no strong signs of active galactic nucleus activity or recent major merger events. The light distribution is concentrated towards the center with a gradual fading towards the edges.
