The galaxy appears as a moderately luminous object with a generally smooth morphology, though some irregularities are visible. Its shape tends towards round, but is slightly off from perfectly circular. The galaxy exhibits a color gradient, with a central region appearing more yellowish-orange, potentially indicating an older stellar population. Fainter, bluer regions are present within the galaxy, which may indicate ongoing star formation. There are signs of minor disturbances that could indicate an ongoing or past interaction with another galaxy. The overall structure suggests a disk galaxy, likely a spiral galaxy observed at an angle, with a central bulge. 
