The galaxy presents as a spiral type, characterized by a central bulge and a prominent disk. The bulge appears moderately sized relative to the overall galaxy dimensions. Spiral arms are clearly visible, displaying a winding pattern.

The dust lanes within the spiral arms are also somewhat pronounced, contributing to the galaxy's structured appearance. There is a notable presence of HII regions scattered throughout the spiral arms, indicative of ongoing star formation activity.

The overall color of the galaxy suggests a mix of stellar populations, with some regions exhibiting bluer hues associated with younger stars. The galaxy does not show signs of major disturbances or a recent merger event, though there may be some minor asymmetry in the spiral arm structure. The galaxy disk does not appear to be edge-on; it is more face-on.
