This galaxy appears to be a relatively compact object with a smooth, somewhat elliptical morphology. The light distribution suggests a centrally concentrated bulge component. There is a subtle blue tint, indicating the presence of some young stars or ongoing star formation, although it appears to be at a low level. There is a slight asymmetry, possibly indicating minor interactions or disturbances. No prominent spiral arms or dust lanes are visible. Overall, it likely consists of a mix of older stellar populations and a small fraction of younger stars, with an estimated mass range from 10^9.6 to 10^9.7 solar masses.
