The object presents as a spiral galaxy, observed at a slight incline to our line of sight. The spiral structure is prominent, with two clear arms emanating from a central bulge. The arms are tightly wound, displaying a relatively smooth texture. The bulge dominates the central region, exhibiting a yellowish hue indicative of an older stellar population. A bar-like structure appears to traverse the central region, exhibiting a moderate presence. Evidence of ongoing star formation is suggested by subtle bluish tinges within the spiral arms. There is a notable absence of significant dust lanes, which contributes to the galaxy's smooth overall appearance. Overall morphology suggests a quiescent, relatively massive system undergoing moderate star formation. No major mergers are occurring.