The galaxy presents as a generally smooth object with a slight elongation, approximating a cigar shape. A bright, concentrated central region is visible, likely indicating a significant bulge component. The light profile appears to fade gradually from the center towards the edges. There is very little evidence of spiral arm structure or distinct dust lanes; it appears to be either an elliptical galaxy or a lenticular galaxy seen at an oblique angle. Based on its color and shape, it is likely a relatively massive galaxy with a low star formation rate. There appears to be no major ongoing merger events, but there may be some very minor disturbances in the outer halo. The color suggests the galaxy is at a moderate redshift.
