The galaxy appears as a centrally concentrated, relatively smooth object. It exhibits an elliptical morphology, with a high degree of roundness. No distinct spiral arms or prominent features such as dust lanes are visible in this image. The galaxy's color suggests a population of older stars, indicative of minimal active star formation. There is no obvious visual evidence of ongoing or recent major merger events. It is likely a relatively massive galaxy, with a high proportion of its stellar mass concentrated in the bulge. Possible minor disturbances cannot be ruled out.
