The galaxy presents as a single, relatively smooth structure. It is elliptical in shape, appearing mostly round. The central region exhibits a concentrated brightness, with the luminosity appearing to decrease gradually towards the outer edges. The galaxy appears to have a yellow hue, which indicates an older stellar population. There are no prominent features that suggest active star formation or significant dust lanes. There are no signs of spiral arm structures, tidal tails, or significant morphological disturbances, suggesting it is likely not undergoing a major merger event. The outer edges appear somewhat ill-defined, fading into the background.
