The galaxy presents as an edge-on disk galaxy. A prominent central bulge is visible, exhibiting a smooth, rounded morphology. The disk component appears relatively thin and shows evidence of some internal structure, although the resolution is not sufficient to discern individual spiral arms or star-forming regions. There appears to be a slight warping of the galactic disk. The colour profile of the galaxy indicates a relatively older stellar population, particularly concentrated in the bulge. The bulge's colour is distinctly redder than the disk. There is no evidence of ongoing major merging activity or significant tidal disturbances in the immediate vicinity. Faint traces of a possible minor interaction can be found near one of the 'tips' of the galaxy.
