The galaxy presents as a disk-like system, exhibiting a generally smooth morphology. There is an indication of some structure within the disk. The central bulge appears bright and somewhat distinct. The color profile suggests a population of older stars dominate, but the presence of color variation throughout the disk could indicate a more complex stellar population. It exhibits a moderate size. The galaxy is neither perfectly round nor significantly elongated, presenting an intermediate shape. The overall appearance suggests the galaxy is not currently undergoing a major merger event, although minor disturbances cannot be ruled out from this image alone.
