The galaxy presents as a relatively compact object with an overall elliptical morphology. It exhibits a smooth light distribution, lacking prominent spiral arm structures or significant dust lanes within the observed wavelength range. The core region shows a concentration of light, suggesting the presence of a galactic bulge. The light tapers off gradually towards the edges of the galaxy. The overall color appears to be on the redder side, potentially indicating an older stellar population. There is a lack of evident signs of ongoing major star formation activity. The ratio of the minor to major axis is approximately 0.7, suggesting a flattening.
