The galaxy presents as a spiral type, observed at a moderate inclination relative to our line of sight. The disk component exhibits a structured appearance, with a non-uniform distribution of light. There appear to be at least two prominent spiral arms emanating from the central region, displaying a medium winding. There is evidence of ongoing star formation within the spiral arms, noted by regions of bluer light, indicating the presence of younger, hotter stars. 

The central bulge appears as a concentrated region of relatively uniform yellowish light, suggesting an older stellar population. The bulge component appears to be moderately sized. The galaxy appears to be fairly isolated, showing no signs of recent or ongoing interaction with other galaxies. There is no clear indication of a strong central bar structure. The overall morphology of the galaxy suggests a relatively undisturbed disk galaxy.
