The galaxy exhibits a generally elliptical morphology, viewed nearly edge-on from our perspective. The dust lane is prominently dark, obscuring light from the central bulge which is visible in the image, but not distinctly.

A faint, diffuse halo surrounds the central region, suggesting an extended distribution of stars or gas. Some evidence of tidal tails on the right of the image indicates possible gravitational interactions with another galaxy.

The galaxy appears relatively smooth, with no distinct spiral arm structures visible. There is a slight increase in blue color towards the end of the left arm, possibly indicating a region of active star formation. The galaxy appears asymmetrical, and it is not immediately clear if the galaxy has had recent mergers.
