The galaxy presents as a flattened, disk-like structure, seen at an oblique angle. The central region appears brighter and more condensed, indicative of a galactic bulge. The overall color of the main body leans towards blue, potentially suggesting ongoing star formation. There is a subtle dust lane visible in the disk. One edge appears to have a star-forming region that leans towards a yellow hue, possibly indicative of older stars in that region. The overall smooth appearance suggests a relatively evolved system, though not entirely devoid of star-forming activity. There is no clear evidence of a major ongoing merger, though a slight asymmetry hints at a possible minor interaction in the past. 
