The galaxy presents as a somewhat amorphous, disk-like structure, exhibiting a moderately smooth morphology, with a noticeable central bulge, which is more prominent and appears yellowish, suggesting an older stellar population. The outer regions display a bluer hue, possibly indicating ongoing or recent star formation. There is a slight asymmetry in the galactic disk, with one side appearing somewhat more extended than the other, suggesting a potential gravitational interaction or past merger event. While the galaxy has a primarily centralized form, there are slight hints of disturbances within the galaxy, perhaps hinting at minor tidal distortions. The overall color gradient, from the yellow center to the blue edges, suggests a radial dependence of stellar population age and star formation activity.
