The galaxy presents as a disk galaxy, viewed nearly edge-on. A dust lane bisects the galaxy, obscuring a significant portion of the central bulge. The bulge appears relatively small. The disk component exhibits a smooth texture and consistent color, suggestive of a relatively quiescent star formation environment. No spiral arm structures are distinctly visible, possibly due to the near edge-on orientation and smooth distribution of the stellar population. There are no prominent tidal features or significant signs of interaction with other galaxies. The overall color suggests the presence of a mix of young and old stellar populations with a redder hue dominating.
