The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated luminosity profile, with the brightness decreasing gradually towards the outer regions. The overall color is somewhat red, potentially indicating an older stellar population and a relatively low rate of ongoing star formation. There's little evidence of spiral arms or prominent dust lanes, reinforcing the classification as an elliptical galaxy. The galaxy shows a generally round shape and is not currently undergoing any major merging activity, although some minor disturbances cannot be entirely ruled out based on the image alone.