The galaxy appears as a single, concentrated object with a relatively smooth light profile. The central region exhibits a bright, yellowish hue, suggesting an older stellar population. Fainter, reddish components are observed in the immediate surrounding area. There are no apparent spiral arm structures or significant dust lanes, but there may be a faint disk that is difficult to resolve. The overall shape is close to circular, with only a slight deviation towards ellipticity. There is no strong evidence of ongoing major merger activity, but the faint asymmetry on one side may indicate minor disturbances. 
