The galaxy appears to be an elliptical galaxy, characterized by its relatively smooth and featureless morphology. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades into the surrounding halo. The galaxy has a roughly elliptical shape, with a moderate ellipticity, appearing somewhat rounded but not perfectly spherical. There is no discernible evidence of spiral arms, dust lanes, or active star formation regions within the observed optical wavelengths. The color index suggests a population of older stars, indicating it is likely a passively evolving system with a low star formation rate. There is no obvious sign of any recent or ongoing major merger events, although some minor tidal disturbances or interactions with smaller satellite galaxies cannot be ruled out based on this image alone.
