The galaxy presents as a disk galaxy, seen at a slight inclination from our vantage point. A central bulge appears bright and somewhat spherical, exhibiting a yellowish hue, suggesting an older stellar population concentrated in the core. Faint spiral arm structures are discernible, though not sharply defined. These arms appear bluer in color, indicating ongoing or recent star formation. There is a very slight asymmetry to the galaxy's overall shape, but this might be due to disturbances. The galaxy doesn't appear to be undergoing a major merger currently.
