The galaxy appears to be a relatively smooth, early-type galaxy, likely an elliptical. It presents a centrally concentrated luminosity profile, with the brightest region located at the core. There is a noticeable color gradient, with the central region appearing slightly redder and the outer regions appearing bluer, possibly indicating a population of younger stars in the outer regions compared to an older stellar population at the core. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated but not excessively so. No strong dust lanes or spiral arm features are visible. There may be some evidence of minor disturbances in the galaxy's outer regions, but this is subtle. Overall, the galaxy's morphology suggests a relatively evolved system with a large mass.
