The galaxy presents as an edge-on spiral with a prominent bulge. The bulge appears smooth and spheroidal, with a concentrated luminosity. A faint disk extends outwards, bisecting the bulge, which is difficult to resolve any spiral arm structure within the disk due to the edge-on orientation. The dust lane is visible, indicative of a rotating disk with associated gas and dust. There is an area of low-level star formation. The galaxy exhibits a strong red color, suggesting the presence of an older stellar population and lower levels of recent star formation. The galaxy shows no apparent signs of major mergers or significant tidal disturbances.
