The galaxy presents as an elongated, spindle-shaped structure, viewed at a high inclination. Its color gradient transitions from a yellowish hue at its core to a bluer tinge along the outer edges. The central region appears relatively smooth and concentrated, potentially indicative of an older stellar population. The outer regions show a subtle disk-like structure with some suggestions of faint spiral arms. There is no apparent major disturbance or ongoing merger activity. The overall morphology suggests a possible classification as a spiral galaxy, likely of type Sb or Sc, seen edge-on.
