The galaxy presents as an elongated, disk-like structure. Its color profile suggests an evolved stellar population, exhibiting a yellowish-orange hue, particularly concentrated towards the central bulge. The edges of the disk appear somewhat indistinct, possibly due to lower surface brightness or the galaxy's distance. There is a slight hint of a bluer component at one end of the galaxy, implying possible recent star formation, though not pronounced. The overall morphology is relatively smooth with only a few minor disturbances. There is no clear indication of a major merger or significant tidal interaction, although some minor distortion cannot be completely ruled out.
