The galaxy appears to be a spiral galaxy, with a central bulge that appears yellow in color, suggestive of an older stellar population. There are extended faint arm structures. The arms appear to be of a bluer hue, possibly indicative of ongoing star formation within these regions.

The galaxy has a non-negligible disk, which is not perfectly edge-on, as we can see some features within it. There is evidence to suggest a lack of any strong tidal features or major disturbances in the galaxy's morphology. This may suggest the galaxy has not undergone a major merger in its recent history. 

The galaxy is relatively large and luminous.
