The galaxy presents as a disk galaxy, viewed at an oblique angle. A prominent central bulge is visible, exhibiting a yellowish hue, indicative of an older stellar population. Spiral arm structures are present; however, they appear somewhat indistinct, and lack well-defined boundaries. The dust lanes are also subtle and not particularly prominent. The galaxy appears relatively smooth, with no obvious signs of major mergers or significant tidal disturbances. Overall, the galaxy appears to be relatively quiescent with a moderate inclination.
