The galaxy presents as a concentrated, largely featureless spheroid. The central region exhibits a yellowish hue, potentially indicating an older stellar population. There is very little indication of spiral arm structure or significant dust lanes. The galaxy appears relatively smooth, with no discernible major distortions suggesting an ongoing merger. There is slight asymmetry between the major and minor axis. The overall morphology suggests that this is likely an elliptical galaxy. There may be some minor disturbance present, given the faint, slightly elongated, fuzzy morphology that is present.