The galaxy presents as a relatively smooth and centrally concentrated object. The light distribution exhibits an elliptical morphology with a high degree of central concentration. There is a lack of prominent spiral arm structures or a distinct bulge; instead, the luminosity appears to gradually decrease from the core outwards. The galaxy's color index appears to be moderate, with a slight tendency towards the redder part of the spectrum. This is suggestive of an older stellar population and a lower rate of current star formation. The overall structure does not indicate any major recent merging events or significant tidal disturbances. It can be approximated that its isophotal shape is somewhat elliptical, deviating slightly from a perfect circle.
