The galaxy presents as a spiral galaxy, observed at a high inclination relative to our line of sight. The central bulge appears moderately prominent, exhibiting a yellowish hue indicative of an older stellar population. Two distinct, tightly wound spiral arms emerge from the bulge, tracing a clear path around the galaxy. Star formation appears active within these arms, as evidenced by localized areas of bluish emission. The overall structure shows no obvious signs of a major merger event, although subtle irregularities in the outer disk may suggest minor gravitational disturbances. A subtle bar feature crosses the central bulge of the galaxy.
