The galaxy appears to be a spiral galaxy with a relatively bright central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. Fainter spiral arms extend outward from the central bulge, displaying a loose winding pattern. The arms are somewhat clumpy, potentially indicating active star formation regions. A subtle bar structure may be present, though it is not strongly defined. The galaxy's disk is oriented at a slight angle relative to our line of sight, but mostly face-on. There is no indication of any major ongoing merger events, though some minor distortions could be present.