The galaxy presents as a somewhat elliptical, relatively smooth object. Its central region exhibits a high concentration of luminosity, suggesting a prominent galactic nucleus. The color profile indicates a generally older stellar population, appearing redder in hue, which could be indicative of reduced star formation activity within the galaxy. There's a noticeable absence of well-defined spiral arms or significant dust lanes. The overall form suggests it is an early-type galaxy, potentially an elliptical or lenticular galaxy, with a minor possibility of past merger activity.
