The galaxy appears as a relatively small, edge-on disk galaxy. A prominent central bulge is visible, exhibiting a smooth, somewhat elliptical profile with a yellow-orange hue, suggestive of an older stellar population. The disk is thin and elongated, displaying a similar color to the bulge. The galaxy exhibits faint signs of disturbance in the disk, possibly from minor interactions, but the structure is largely intact. Based on the color, one can roughly assume that there may be a high degree of past star formation, but the current star formation is relatively low. The bulge appears to be mostly rounded.
