The galaxy presents as a relatively smooth, centrally concentrated object. It appears largely elliptical in shape, with an approximate diameter of 5.4 kpc. The galaxy's core exhibits a bright, slightly blue-shifted region, possibly indicating the presence of ongoing or recent star formation. Moving outwards from the center, the light becomes redder suggesting an older stellar population. There is some evidence of minor tidal disturbances or interactions, possibly from a minor merger event in the recent past.
