The galaxy presents a generally smooth morphology, lacking any prominent spiral arms or a distinct disk-like structure. It appears to be largely spheroidal in shape, with a high degree of central concentration of light. The color profile seems to be redder in the central regions, potentially indicating an older stellar population. A slightly bluer halo can be seen, suggesting some recent, but not substantial, star formation activity. There is no apparent evidence of any major mergers or tidal disturbances. The overall light distribution is quite symmetrical, suggesting a relaxed system.
