The galaxy presents an approximately circular morphology, exhibiting a centrally concentrated luminosity profile. The core region displays a high degree of surface brightness. The overall color appears relatively blue-green, suggesting the presence of a moderate population of younger, hotter stars or active star formation regions. The outer regions show some fuzziness, potentially indicating the presence of a faint disk or extended halo component. There is some indication of possible minor disturbances to the overall shape, however, a merger is unlikely. A smooth morphology seems to be a major component of the galaxy, however, there is likely also a faint disk.
