The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The core exhibits a bright, nearly circular appearance. There is a slight elongation or flattening to the overall shape. It is a disk galaxy, with a distinct color gradient between the core and the outer regions, suggesting differing stellar populations and possibly ongoing star formation. The central region shows a somewhat yellower-redder hue, possibly indicative of older stars. The outer regions appear bluer, suggestive of younger stars. There are some slight disturbances present that suggest the possibility of minor gravitational interactions.
