The galaxy presents as a disk galaxy, likely a spiral, viewed at a moderate inclination. The central bulge appears prominent and displays a yellowish hue, suggesting a population of older, redder stars. This contrasts with the bluer tinge observed in the surrounding disk, indicating the presence of younger, hotter stars formed from ongoing or recent star formation. 

The disk itself does not appear to have well-defined spiral arms; it exhibits a more flocculent, patchy structure. The light distribution suggests a relatively high mass galaxy that is actively forming stars. There are subtle signs of a minor disturbance or tidal interaction on the outskirts of the galactic disc.
