The galaxy presents as a disk-shaped structure, elongated along its major axis. A bright, concentrated central bulge is apparent, exhibiting a luminosity gradient towards the core. The disk component shows some evidence of spiral arm structure, albeit somewhat irregular.

The colors across the galaxy vary. The central bulge appears generally bluer, suggesting a younger stellar population or active galactic nucleus. The spiral arms exhibit a mix of colors, with regions showing bluer hues indicative of ongoing star formation. There is a clear presence of dust lanes or obscuring material particularly within the disk, causing a mottled appearance.

The outer regions of the disk are less well-defined, with a diffuse halo extending beyond the main body of the galaxy. There are faint indications of tidal features or disturbances suggesting possible interactions or past merger events.