The galaxy appears as an elongated, elliptical shape. The light distribution is relatively smooth, suggesting a lack of prominent spiral arms or distinct features. The color gradient indicates a redder core region, likely dominated by older stellar populations, with bluer hues towards the outer edges, which may indicate regions of recent or ongoing star formation. The elongated morphology suggests it may be a lenticular galaxy, possibly transitioning between a spiral and an elliptical form. The galaxy is not perfectly symmetrical, exhibiting a slight warping or distortion, this could be due to interactions with its galactic environment.
