The galaxy presents as an elongated, disk-like structure oriented close to edge-on relative to our line of sight. A central bulge region appears brighter and slightly more yellow/orange-tinged, suggesting an older stellar population concentrated towards the center. The outer disk fades in intensity, displaying a bluer hue, indicative of ongoing or recent star formation. There is some evidence of tidal streams, though they are not very visible.

The galaxy's morphological classification is likely a spiral or lenticular galaxy, given its disk-like appearance. The ratio of disk-to-bulge luminosity seems to favor the disk, though the edge-on orientation makes precise assessment challenging. There's a slight asymmetry in the outer disk's appearance, suggesting a possible minor interaction with another galaxy or recent merger event which can be seen through the tidal streams. Overall, it is likely that we are looking at a galaxy of intermediate mass with moderate levels of recent star formation.