The galaxy presents a generally smooth morphology, with a centrally concentrated luminosity profile. There is a hint of a disk-like structure, but no clear spiral arms or bar are visible. The dominant color is bluish, suggesting a stellar population with ongoing or recent star formation. There are no apparent signs of major mergers or significant tidal disturbances, though minor disturbances cannot be ruled out. The galaxy appears to be somewhat rounded in shape, neither perfectly spherical nor highly elongated. Given its luminosity, the galaxy is likely of intermediate mass. The relatively high star formation rate suggests it is not a quiescent galaxy.
