The galaxy presents as a somewhat elongated, though largely smooth, structure. A bright, concentrated central bulge is visible, with the luminosity decreasing towards the outer edges. The color appears yellowish-white in the central region, suggesting an older stellar population dominates the core. There is a hint of bluer hues in the faint outskirts, potentially indicating regions of more recent star formation, but this is subtle. The disk appears to be at an inclined angle relative to our line of sight. Overall, the galaxy exhibits minimal signs of significant disturbance or recent major mergers, though a minor asymmetry cannot be ruled out.
