The galaxy presents as a smooth, elliptical structure. Its overall color profile appears to be predominantly yellow-orange, with a more intense concentration of this color toward the center, suggesting an older stellar population dominating the galactic core. There appears to be very little evidence of distinct spiral arm structures or prominent dust lanes. The observed shape indicates a generally round form, though it exhibits a slight elongation. Based on the color profile, the galaxy's estimated mass range suggests that star formation activity is low, possibly due to gas depletion or feedback mechanisms. Though largely smooth, there might be some minor disturbances or interactions occurring given the slight elongation of the shape. The overall appearance of the galaxy suggests that it is likely a mature galaxy transitioning to a more passive state of stellar evolution.
