The object presents as a spiral galaxy, observed nearly edge-on. A prominent central bulge is visible, exhibiting a bright, concentrated luminosity. A faint, extended disk is observable, lending to the galaxy's overall elongated morphology. The galaxy's disk appears relatively smooth with no prominent or knotty star forming regions. A slight blue tinge suggests ongoing, albeit moderate, star formation within the galaxy. There is no morphological evidence of a major merger event or tidal disturbance, and the galaxy looks isolated and undisturbed.
