The galaxy presents as a relatively small, edge-on disk galaxy. It exhibits a concentrated central bulge that appears yellowish-white, suggesting a population of older stars and a low rate of current star formation within the bulge. The disk component shows a faint, bluish hue, potentially indicating the presence of younger stars and ongoing star formation, although the color is not pronounced, suggesting a modest rate. The dust lane is visible in the image, and the galaxy has no major disturbances or a companion galaxy nearby. Overall, the galaxy appears to be a relatively undisturbed, mature spiral galaxy.