The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape. Its light profile suggests a high degree of central concentration, with a bright, compact core gradually fading towards the outer regions. The observed color appears largely uniform and red-shifted, suggesting an older stellar population and potentially reduced levels of ongoing star formation within the galaxy. There is no obvious evidence of spiral arm structures, dust lanes, or significant tidal disturbances, indicating a dynamically relaxed system. The galaxy's round appearance suggests a minimal degree of inclination from our line of sight. There are no obvious signs of recent or ongoing merger activity, the galaxy appears largely undisturbed.
