This galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. There is little evidence of spiral arm structure or significant dust lanes, and its overall shape approximates a circle. The galaxy exhibits a generally even distribution of light across its surface. The color of the galaxy appears to be slightly redder, suggesting an older stellar population with relatively little ongoing star formation. There are no obvious signs of recent major merger events, though a very slight asymmetry or minor disturbance in the galaxy's outer regions could indicate past interaction, though this is not clearly visible. The galaxy's light profile suggests a gradual decrease in brightness from the core to the outer edges, consistent with a bulge-dominated system.
