The galaxy appears to be a spiral, viewed at a moderate inclination. There's evidence of spiral arm structure, though not highly defined. The central bulge appears moderately prominent, with a yellowish hue suggesting an older stellar population. Some blue regions are observed within the disk, potentially indicating regions of active star formation. The overall structure doesn't show any major signs of disturbance or interaction with another galaxy, although there may be minor asymmetry. A bar structure may be present. The galaxy has a relatively smooth appearance overall.
