This galaxy exhibits an elliptical morphology, appearing as a smooth, elongated spheroid. The light profile suggests a concentrated central bulge, fading gradually outwards. The color gradient indicates a slightly bluer hue in the outer regions compared to the yellowish core. There is no discernible spiral arm structure or dust lane features visible. The overall appearance points towards a passively evolving galaxy with a substantial population of older stars and relatively low current star formation activity. There is no major disturbance or interaction with other galaxies noted.
