This galaxy presents a morphology that appears predominantly smooth. Its overall shape is somewhat rounded, though it leans towards being an intermediate shape rather than perfectly circular. There is a slight elongation along a single axis. The galaxy exhibits a central region of higher intensity, possibly indicating a concentration of older stars or a galactic bulge. Faint hints of spiral structure or tidal disturbances cannot be ruled out, though the image quality makes these features difficult to ascertain definitively. The blue hue suggests recent or ongoing star formation, especially when considering its size which is approximately 6 kpc in radius. Any signs of interactions or mergers appear to be minor if present. Overall, the galaxy appears to be a relatively isolated system in an intermediate stage of evolution.
