The galaxy presents an elliptical morphology, appearing as a flattened spheroid with a high degree of central concentration. Its light profile is generally smooth, lacking any prominent spiral arm structures or distinct features indicative of active star formation regions. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a redder periphery. This suggests a stellar population dominated by older, cooler stars in the outer regions, with a possible presence of younger, hotter stars towards the center. The orientation of the galaxy reveals that it is viewed at an oblique angle, with its major axis extended horizontally across the image. No signs of tidal disturbances, mergers, or interactions with neighboring galaxies are clearly visible.
