The galaxy appears to be a spiral galaxy viewed at a slight angle. It exhibits a prominent central bulge that is relatively smooth and concentrated, appearing yellowish in color, indicating an older stellar population. Extending outward from the bulge, there are hints of spiral arms that seem somewhat clumpy and less well-defined. These arms show some blueish coloration, suggesting the presence of younger, hotter stars and ongoing star formation. There also appears to be a slight disturbance in the morphology of the spiral arms, possibly due to a minor interaction with another galaxy, although no distinct companion galaxy is apparent in this image. The dust lanes within the spiral arms are not clearly visible, indicating a relatively low dust content in the galaxy. The galaxy is approximately 4.5 kiloparsecs in radius and is relatively faint.
