The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a moderate level of radial symmetry, although it is not perfectly circular. There is a slight elongation, indicating a possible cigar shape. The galaxy exhibits a color gradient, with the central region appearing more yellowish-orange and the outer regions trending towards a slightly bluer hue. This suggests that the central region is dominated by an older stellar population, while there might be some ongoing star formation or a younger population in the outskirts. No prominent spiral arms or dust lanes are visible, supporting the classification as a relatively smooth galaxy. There is no obvious evidence of a major merger or significant tidal disturbances, although a faint, minor asymmetry cannot be ruled out based on this image alone.
