The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a color gradient from a slightly bluer core region to redder outer regions. Its overall form appears elliptical or lenticular, with no obvious spiral arm structures detected. There is, however, a very minor hint of a possible disk component. The concentration of light suggests a relatively old stellar population, particularly in the outer regions. The absence of clear dust lanes or active star-forming regions further supports this conclusion. The galaxy appears undisturbed, with no significant signs of ongoing or recent mergers or tidal interactions. 
