The galaxy presents as a single, relatively smooth object, with minimal discernible substructure. It appears largely spheroidal in shape, exhibiting high degree of roundness with a concentrated central bulge. Color gradients suggest a predominantly older stellar population, with the central regions appearing more yellowish, possibly indicating a higher concentration of evolved stars. There is little evidence of active star formation based on the absence of prominent blue regions. The galaxy does not show any signs of ongoing major mergers or significant tidal disturbances in this image, however there is a small amount of disturbance in the bottom left corner of the galaxy, there is no indication of a distinct disk component.
