This galaxy presents a largely featureless, elliptical morphology. It exhibits a smooth, almost perfectly round structure with no discernible spiral arms or bar. The galaxy's light is centrally concentrated, displaying a bright, yellowish core that gradually diffuses into the surrounding halo. There is a notable lack of distinct dust lanes or prominent star-forming regions. The overall color suggests an older stellar population, consistent with a low star formation rate. There is no visual evidence of any ongoing major merger events, although minor disturbances cannot be ruled out at this resolution. The galaxy appears to be relatively isolated within its field.
