The galaxy presents a generally smooth, though not perfectly elliptical, appearance. A centrally concentrated bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population. Fainter, bluish emissions extend outwards, indicating the presence of a galactic disk. While the disk is present, there are no clearly defined spiral arms, suggesting the presence of some disturbances, or perhaps a more flocculent spiral structure. There is no apparent strong bar feature bisecting the central bulge, and the galaxy appears relatively isolated, showing no signs of ongoing major mergers or significant tidal disturbances in its morphology. The disk appears neither perfectly face-on nor edge-on, instead lying at an angle to our line of sight, but closer to face-on than edge-on.
