The galaxy presents a smooth, elongated morphology, appearing cigar-shaped in its overall form. The light distribution suggests a bulge-dominated system, possibly an elliptical galaxy. There is little evidence of spiral arm structure or significant dust lanes. The color is primarily redder, indicating an older stellar population and low levels of ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger event, though a possible minor disturbance cannot be ruled out. The galaxy displays a somewhat diffuse appearance at this resolution, with light that appears very compact.
