The galaxy presents as a relatively faint, elongated structure. It appears to be a spiral galaxy viewed at a high inclination, nearly edge-on. A central bulge is subtly discernible, exhibiting a yellowish or reddish hue, suggestive of an older stellar population. Extending from the bulge are faint, blueish arms. These arms show some degree of asymmetry, possibly indicative of tidal interactions or past mergers. There appears to be an area of active star formation visible, indicated by the blue color in one of the arm segments. The galaxy does not show any signs of a major ongoing merger or significant tidal disruption. The overall morphology suggests a disk galaxy with a relatively smooth appearance but some signs of disturbance.