The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution suggests a predominantly older stellar population, indicated by the yellowish-red hue. There is little evidence of prominent spiral arms or significant dust lanes. The overall shape is generally round. There is a slight color gradient, with the central region appearing more yellow and the outer regions subtly more red. No major disturbances or mergers are immediately apparent in the galaxy's structure.