The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a moderate degree of ellipticity, appearing more oval than perfectly circular. No distinct spiral arms or bar structures are discernible within the image. There is a subtle color gradient visible, trending from a slightly bluer central region to somewhat redder outer portions. This could be caused by varying stellar populations. There are no obvious signs of major mergers or significant tidal disturbances. Faint hints of minor irregularities might indicate the presence of ongoing or past interactions, though they are not highly pronounced. The galaxy appears to be of intermediate size and luminosity.
